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Objects below the altitude you select will be considered below the horizon. You can use this to quickly identify objects which - even though technically above zero degrees altitude - are still too low in the sky to be easily observed.
It's usually not worthwhile to observe objects below an altitude of 10 - 15 degrees, since they are lost in atmospheric haze.
This section lists the horizon panoramas that are available in SkySafari. The currently-selected panorama is shown with a check mark. The panorama is only displayed if you've selected Panoramic Image display option above.
Choosing any item from the list of horizon panoramas will automatically select this option! You can create your own horizon panorama - for instance, an image of your own back yard, or your favorite observing site.
You can then import it into SkySafari, to show the sky as it realistically appears from your location. To do this, first create a panorama using your digital camera, and a panorama-stitching program like Adobe Photoshop, Canon PhotoStitch, or DoubleTake for macOS.
Resize your panorama image to dimensions of exactly pixels wide x pixels tall. When you're done photoshopping, save your panorama as a bit RGBA color image file in PNG format.
Make sure your image contains an alpha or transparency layer that accurately indicates the parts of your panorama that are opaque the ground, trees, buildings, etc.
If you are using SkySafari on an iPhone, iPad, or iPod touch, you can import your horizon panorama using iTunes file sharing.
To do this, connect your iPhone or iPad with a USB cable to a computer running iTunes. Select your iOS device when it appears in iTunes, then find the "Apps" section that lists all the apps on your device.
Choose SkySafari from the list of apps. Add your horizon PNG image file to the list of SkySafari Documents displayed by iTunes, or drag and drop it into the list.
If everything works correctly, your image will then appear in the list of horizon panoramas in SkySafari.
You can select and display it just like SkySafari's other built-in horizon panoramas. If your horizon panorama doesn't appear in SkySafari's list, make sure it's in PNG format, and that its name ends with ".
Make sure its dimensions are x , and that's a bit RGBA color image with an alpha transparency layer. If all else fails, you can email your image to Simulation Curriculum technical support, and we can try to debug it for you.
If you are using SkySafari for Android, you can import your horizon panorama using your SD card. To do this, connect your Android device with a USB cable to a computer.
Then mount your Android's SD card on your computer, so it appears as a disk. Look for a SkySafari, SkySafari Plus, or SkySafari Pro folder on the root top level of your SD card, depending on which version of SkySafari you own.
Then copy your horizon PNG image file into the Horizon Panoramas folder within this folder. For example, if you own SkySafari Pro, copy your panorama to the following directory on your SD card:.
The settings in this view control the display of planets, moons, and other "minor bodies" in the solar system asteroids and comets , as well as artificial Earth-orbiting satellites.
Show Planets: Displays planets and moons in the sky chart. Planet grids show the orientation of the planet's equator and rotational axis.
Their north poles are drawn as bold lines; south poles are shown with lighter lines. Note: this option is only available in SkySafari Plus and Pro.
When turned off, planets shown as fully illuminated, without any night side shading. To see these objects' surfaces unobscured by clouds, turn off this option.
This option can slow performance when zoomed in a planet's disk, but generates a very pretty view. Spacecraft that have landed on other solar system objects, and cities on Earth, are indicated with a green dot and label.
Only the largest features are labelled when a planet's disk appears very small; to see more labels for smaller features, zoom in on the planet.
All of these are small, asteroid-sized objects that are only visible in large professional telescopes. Note: this option is only available in SkySafari Pro.
Show Planet Orbits: Shows orbital paths of the major planets around the Sun. Since the planets orbit in the nearly the same plane as the Earth the Ecliptic plane , their orbits appear near the Ecliptic line - the Earth's orbit as seen from the Earth - in the sky.
Show Moon Orbits: Shows orbital paths of the moons around their primary parent planet. You may need to zoom in on a planet to see its moon orbits; Mercury and Venus have no moons!
Selected Object Orbit: Shows the orbit of the selected planet, moon, asteroid, comet, or satellite. You need to select such an object and turn on this option to show its orbit.
Selected Object Path: Shows the apparent path of a solar system object across the sky, with its position at specific dates labelled. The solar system object must be selected, and you must be viewing it from the Earth's surface, in order to see the path.
When this option is turned on, the Earth's or Moon's umbral and penumbral shadows are shows as concentric circles.
Inside the smaller umbral shadow, the Sun is totally hidden; inside the larger penumbral shadow, the Sun is only partially blocked.
This can be helpful for simulating lunar and solar eclipses, and illustrating the difference between total and partial eclipses.
Magnitude Limit: This item lets you set the faintest planets, moons, asteroids, comets, and spacecraft that the sky chart will display.
You can use this item to filter out the many hundreds of faint asteroids and comets that are not observable in backyard telescopes - or you may want to show them all!
Planet Magnification: This slider lets you magnify the Solar System's major planets by a factor of up to 10,x their true size. The planets are very small compared to the space between them.
This option is useful for showing comparative views of the planets from different perspectives. Moon Magnification: This slider lets you magnify the moons of the planets by a factor of up to x over their true size.
Since most moons are very small compared to their primary planet, this option lets you exaggerate them to make easier comparative views.
SkySafari normally updates its database of asteroid, comet, and satellite orbits once per week. In SkySafari Plus and Pro, you can tap this button to download new asteroid, comet, and satellite orbit data any time your iOS or Android device is connected to the internet.
SkySafari will download the following files:. These downloads should take 10 - 30 seconds if you are connected to the internet by Wi-Fi, and a 1 - 3 minutes if you are connected by a cellular data network.
If successful, SkySafari will report the number of asteroid, comet, and satellite orbits that it has updated. If that number is zero, it probably means SkySafari can't connect to the on-line data sources for this information because the server is down, or because you are not connected to the internet, etc.
Updating your orbit data every month or so is a good idea. It will ensure that SkySafari's position predictions are accurate.
This is especially true for satellites, whose orbits change rapidly due to atmospheric drag, and due to perturbations from the Earth's non-spherical gravity field.
Updating also ensures that as new objects are launched - or discovered! The settings in this view let you control the display of stars, including the number of stars that will be shown, the size and color of the star symbols, and the labelling of stars with their names or catalog numbers.
Show Stars: Sets whether stars are displayed in the sky chart. When turned off, most of the other settings in this view are disabled. Magnitude Limit: Sets the star magnitude limit.
This determines the faintest stars that are visible in the sky chart. The brighter a star, the lower its magnitude.
The faintest stars visible to the naked eye are about magnitude 6. Very bright stars can have negative magnitudes; the brightest star in the sky, Sirius, is magnitude The magnitude limit will change automatically as you zoom the sky chart in and out.
When zoomed in, fainter stars are displayed. Proper Names: Sets whether proper names are displayed for stars when possible.
When turned off, stars' names are displayed using their catalog numbers e. Greek Symbols: Sets whether greek symbols are displayed for stars which have Bayer letters.
When turned off, greek letters are spelled out in English, e. Name Density: Sets the percentage of stars whose names are displayed on the sky chart.
Double Stars: displays double stars with their component identifiers A, B, C, D, etc. For binary stars with known orbits, this option also displays the orbital path of the secondary component relative to the primary.
Turn this option on, then zoom in on Sirius or Alpha Centauri, and take a look! Symbol Size: Sets the size of the star symbols.
Use small, subtle star symbols to give the screen the appearance of the night sky. Color Intensity: Sets the displayed intensity of the color difference between stars of different spectral types.
The settings in this view let you control the display of star cluster, nebulae, and galaxies - including the selection of deep sky objects that are shown, and the labelling of objects with their names or catalog numbers.
Show Objects: Draws symbols for star clusters, nebulae, and galaxies in the sky chart. Show Images: Displays images of deep sky objects in the sky chart.
When turned on, Digitized Sky Survey images of several hundred best-known deep sky objects are drawn at their true size and orientation in the sky chart.
Deep sky images can be displayed independently of deep sky object symbols above , and vice-versa. Best-Known Only: Sets whether only the best-known deep sky objects are shown in the sky chart.
These objects include the Messier objects, the Caldwell objects, and any other deep sky objects with a proper or common name.
The Messier Catalog is a famous list of prominent deep sky objects compiled by the 18th century astronomer Charles Messier. The Messier catalog includes some of the most prominent star clusters, nebulae, and galaxies visible from the northern hemisphere, such as the Hercules Cluster M 13 and the Whirlpool Galaxy M The Caldwell Catalog is a modern complement to Messier's list, compiled in by the British astronomer Patrick Caldwell-Moore.
It includes additional "Messier-quality" deep sky objects which Messier missed, many because they are only observable from the southern hemisphere.
Together, the Messier and Caldwell lists include most of the deep sky objects easily visible in backyard telescopes from both hemispheres.
Show in Wide Fields: allows deep sky objects to be displayed when the field of view is wider than 45 degrees. This option is turned off by default, since deep sky objects can only be seen through binoculars or telescopes, which have very small fields of view.
However, turning this option on may let you see the distribution of for example galaxies across wide areas of the sky. Magnitude Limit: Sets the deep sky object magnitude limit.
This determines the faintest deep sky objects that are visible in the sky chart. The brighter an object, the lower its magnitude.
When zoomed in, fainter objects are displayed. Intensity: Sets the brightness used to display deep sky object symbols and names.
Show Names: Sets whether deep sky objects' names are displayed next to the objects in the sky chart.
Proper Names: Sets whether proper names are displayed for deep sky objects, when possible. When turned off, deep sky objects names are always shown using catalog numbers e.
Name Density: Sets the percentage of deep sky objects whose names are displayed on the sky chart. Globular Clusters: Sets whether globular clusters are displayed in the sky chart.
These are dense concentrations of stars, typically containing tens of thousands to millions of stars. These massive clusters are among the oldest objects in our galaxy.
Examples are M 13 in Hercules and M 22 in Sagittarius. Bright Nebulae: Sets whether bright nebulae are displayed in the sky chart. These are glowing clouds of gas usually found in the disk of the Milky Way.
These nebulae glow either from the reflection of light from nearby stars or from the emission of light produced by nearby stars heating the nebulae.
Examples are M 42 the Great Orion Nebula in Orion and M 20 the Trifid Nebula in Sagittarius. Dark Nebulae: Sets whether dark nebulae are displayed in the sky chart.
These are opaque clouds of cold dust which obscure the light from the stars behind them. They are mostly located along the Milky Way.
Examples are B 33 the Horsehead Nebula in Orion, and the Coal Sack in Crux. Planetary Nebulae: Sets whether planetary nebulae are displayed in the sky chart.
These are expanding shells of gas expelled from a star late in its life. A round, planet-like appearance led to the name "planetary nebulae" in the eighteenth century, though there is no actual connection with planets.
Examples are M 57 the Ring Nebula in Lyra and M 27 the Dumbbell Nebula in Vulpecula. Galaxies: Sets whether galaxies are displayed in the sky chart.
Galaxies are immense star systems outside of our own Milky Way galaxy; many are larger than our own. The total number of galaxies is in the billions, and they extend to the edge of the known universe.
Most galaxies are classified as spiral galaxies, elliptical galaxies, or irregular galaxies, based on their appearance. Examples are M 31 spiral in Andromeda, M 87 elliptical in Virgo, and the Small Magellanic Cloud irregular.
The Milky Way is the visible concentration of stars, star clusters, bright gas clouds, and dark dust lanes that lie along the plane of our galaxy in the sky.
The settings in this view control how the Milky Way is displayed in the main sky chart. Show Milky Way: Turns the Milky Way off or on.
When turned off, the Milky Way is not drawn, and most of the other settings in this section are disabled.
This full-sky H-alpha map is a composite of the Virginia Tech Spectral line Survey VTSS in the north and the Southern H-Alpha Sky Survey Atlas SHASSA in the south.
The view shows the distribution of glowing ionized hydrogen gas clouds in our galaxy's star-forming regions. The colors in this image represent specific wavelengths of infrared light.
Cyan blue-green represents light emitted predominantly from stars and galaxies at a wavelength of 3. Green and red represent light mostly emitted by dust at 12 and 22 microns, respectively.
Galactic dust clouds are visible at these wavelengths. Constructed from observations of the sky at wavelengths spanning microns to 1 cm GHz to 30 GHz.
The Haslam MHz map is derived from 4 separate surveys. In this 3-color image, red is 0. This view shows how the sky appears at energies greater than 1 billion electron volts GeV according to five years of data from NASA's Fermi Gamma-ray Space Telescope.
For comparison, the energy of visible light is between 2 and 3 electron volts. Please Note: The options to show the Milky Way in Hydrogen Alpha thru Gamma Ray wavelengths are only available in SkySafari Pro.
Intensity: Sets the brightness level of the Milky Way when shown as a filled area or realistic image. Fade in Small Fields: When turned on, the Milky Way's intensity will fade to zero as the field of view decreases from 10 to 1 degrees wide.
It is often not useful to show the Milky Way in very small fields of view. The settings in this view let you show or hide grids which display the major celestial coordinate systems, as well as the reference lines and points that those systems are based on.
Show Grid: Sets whether a celestial coordinate grid is displayed on the sky chart. When turned on, the following items are enabled:.
Celestial Equator: Sets whether the celestial equator is displayed on the sky chart. The celestial equator is the plane of the Earth's equator projected onto the celestial sphere.
Galactic Equator: Sets whether the galactic equator is displayed on the sky chart. The galactic equator is the plane of the Milky Way galaxy projected onto the celestial sphere.
Ecliptic Path: Sets whether the Ecliptic path is displayed on the sky chart. The Ecliptic is the plane of the Earth's orbit projected onto the sky.
It is also the annual path of the Sun around the celestial sphere. Meridian Line: Sets whether the meridian is displayed on the sky chart.
The meridian is the projection of your longitude on Earth onto the celestial sphere. It extends from the northern horizon through the zenith to the south cardinal point on the horizon.
An object is said to transit when it crosses the meridian. Celestial Poles: Sets whether the celestial poles are displayed on the sky chart.
The celestial poles are where the Earth's polar axis i. The north and south celestial poles are currently in the constellations Ursa Minor and Octans, but they move slowly over the centuries due to precession.
Galactic Poles: Sets whether the galactic poles are displayed on the sky chart. The north and south galactic poles are where a line perpendicular to the plane of the Milky Way galaxy intersects the celestial sphere.
They are currently located in the constellations Coma Berenices and Sculptor, respectively. Ecliptic Poles: Sets whether the ecliptic poles are displayed on the sky chart.
The ecliptic poles are where a line perpendicular to plane of the Ecliptic intersects the celestial sphere. The north and south ecliptic poles are in the constellations of Draco and Dorado, respectively.
This marks and labels the points directly overhead and underneath your feet. Settings Files let you save all of your sky chart options so you can restore them at a later date.
You can email settings files to yourself, or send them to your friends, so that you or they can easily reproduce a sky chart which you have created.
To do all of these things, select the Save and Restore Settings item from the main Settings view. Default Settings: SkySafari creates a default settings file the first time you run the app.
This settings file is called "Default Settings", and it contains a "snapshot" of the app the first time it was launched. You can restore SkySafari to its initial state at any time by choosing this settings file.
To create your own settings files, tap the "Save New Settings File" button. SkySafari will make another "snapshot" of all the app's current settings, and save them as a settings file called "Current Settings.
You can edit the settings file name to something else if you want a more descriptive title. Description: SkySafari generates a default description for your settings file, to give you an idea of what's inside it.
You can edit this description as well. When you are satisfied with the name and description, tap the "Done" button in the upper right side of the status bar to return to the list of settings files that you have already saved - your new settings file is added to the list!
To restore a saved settings file, tap its name in the list of settings files. SkySafari will display the file's description, to let you make sure this is the file you want.
If so, tap the "OK" button - and all of the app's settings will be replaced with those from the settings file. You can tap the "Cancel" button if you don't want to do this!
You can view and edit a previously-saved settings file's name and description by tapping the small blue arrow to the right of the file's name.
You can overwrite the settings inside the file with a copy of the app's current settings, by tapping the "Update with Current Settings" button.
You might want to do this if, for example, you wanted to tweak the settings inside that file, without having to save them to an entirely new file.
You can email a saved settings file to yourself, or to anyone else, by tapping the "Email This Settings File" button. When the email is received, the e-mail app on the recipient's phone will launch their copy of SkySafari, import the settings file into their list of saved settings, and let them restore the settings you sent them - all in a single step!
Then tap and drag the "grip" icon on the right side of the settings file to move it around the screen. Tap and drag the - minus icon on the left side of the settings file to delete it.
Then tap the settings file you want to move or delete. To do this, connect your iPhone or iPad to a computer running iTunes with a USB cable. To export a settings.
You can also rename or delete observing lists here. Changes should be reflected immediately in SkySafari's Save and Restore Settings section.
To import a settings. If everything works correctly, your settings file will then appear in SkySafari's Save and Restore Settings section. If your settings file doesn't appear in SkySafari, make sure it's a valid SkySafari settings file, and that its name ends with ".
If all else fails, you can email your settings file to Simulation Curriculum technical support, and we can try to debug it for you.
Android users can import and export settings files to SkySafari using their SD card. Look for a SkySafari , SkySafari Plus , or SkySafari Pro folder on the root top level of your SD card, depending on which version of SkySafari you own.
Then locate the Saved Settings folder within this folder. For example, if you own SkySafari Pro, your observing lists are stored in the following directory on your SD card:.
You can also rename or delete settings files directly on your SD card. If everything works correctly, your observing list will then appear in SkySafari's Save and Restore Settings section.
You can select and apply the new settings file, just as any other. If all else fails, you can email your observing list to Simulation Curriculum technical support, and we can try to debug it for you.
SkySafari 5 Plus and Pro allow you to store observing lists and saved settings files in the cloud so they will be available and up to date on all your devices.
Note: Cloud storage is only available in SkySafari Plus in Pro. It's not available in the basic version.
You enable cloud syncing from the Storage settings panel. You may choose to store the files locally, on iCloud Drive or on Google Drive.
The later option should be chosen if you run SkySafari on both iOS and Android devices and want files shared between them.
You must have iCloud Drive enabled in your iOS Settings to use iCloud Drive storage. To use storage on Google Drive you must have an active Google account.
SkySafari will ask you to sign into this the first time you use it. Changed files are uploaded to the cloud only when you quit the app or put it into the background.
It can take several minutes for those changes to propagate to your other devices. For iCloud Drive, files that have changed in the cloud should be automatically downloaded to your device any time SkySafari is active.
If a file doesn't appear to be downloading, try putting SkySafari in the background and then bring it to the foreground again. For Google Drive, files are downloaded each time SkySafari is brought to the foreground.
File conflicts can occur if the same file is modified on two devices within a short amount of time or when you don't have internet access on one or both devices.
Conflicts are resolved by choosing the most recent modification. The two sets of changes will not be merged.
The DSS Cache Storage setting controls how much space is allotted to storing Deep Sky Survey images downloaded from the Object Info view. When the allotted storage is filled, older images are automatically discarded.
Use these settings to specify what kind of telescope hardware you have, and how SkySafari should communicate with your telescope. SkyFi - a Wi-Fi adapter that relays wireless communication from your mobile device to the serial port on your telescope.
Android devices must support Ad Hoc Wi-Fi networks to use our SkyFi wireless adapter; most do not. All iOS devices support Ad Hoc Wi-Fi, and therefore can use SkyFi.
SkyWire - a serial cable accessory for iOS devices. Does not work with Android devices. Does not work with iOS devices.
Note that when using a Celestron WiFi scope, the telescope setup and control interface will be somewhat different.
This is detailed more below. You can also use our SkySafari software, running on a macOS computer with Wi-Fi and a serial port, as a Wi-Fi-to-serial server.
See Simulation Curriculum's web site at www. Scope Type - selects the type of telescope you want to control.
SkySafari can control any of the telescopes in the list. SkySafari supports many encoder systems that can read out the telescope position but not actually move the telescope.
The Celestron AstroMaster and JMI NGC-MAX are examples of such encoder systems. Mount Type - selects your telescope's type of mounting: Equatorial Push-To - a non-motorized mount whose right ascension axis is pointed at the celestial pole.
The mount must be manually turned around this axis to follow the diurnal motion of the sky. Equatorial GoTo Fork - a motorized equatorial mount that automatically follows the diurnal motion of, and can automatically slew to, targets in any part of the sky.
Has one or two fork arms that suspend the telescope between them. The Meade LX and Celestron NexStar when used with an equatorial wedge are examples.
Equatorial GoTo German - a motorized, polar-aligned mount that requires reversing the telescope tube to the east or west side of the mount when the telescope passes through the meridian.
Examples include the Losmandy and Takahashi mounts. Push-To on Equ. Platform - a non-motorized mount that must be manually pushed to targets in different parts of the sky.
However, it sits on a motorized platform that is aligned with the Earth's polar axis, so the mount follows the diurnal motion of the sky when it is not being pushed.
Push-To - a non-motorized alt-azimuth platform with fork arms that suspend the telescope between them. It is moved manually by pushing the telescope tube.
It sits flat on the ground, so its "up-down" and "left-right" axes of motion align to the local horizon and zenith.
This includes most Dobsonian telescopes. GoTo - a motorized alt-azimuth platform with fork arms that suspend the telescope between them, and can slew to any set of coordinates in the sky on command.
Includes the Meade LX and Celestron NexStar when used in the alt-azimuth configuration. If your telescope mount has encoders which provide a digital readout of the scope's position, additional text fields will appear here.
These let you specify the encoder resolution. Get Automatically - If turned on, SkySafari will attempt to read these values from your encoders when it connects to the telescope controller.
If turned off, you can enter the encoder steps per revolution manually; then SkySafari will send the values you entered to the encoders when connecting to the telescope.
You can do this if for example your mount is using gears or pulleys to increase the effective encoder resolution.
Depending how your encoders are installed, their position readouts may increase when they are turned clockwise, or increase when they are turned counterclockwise.
If the encoder position readouts increase when they are turned counterclockwise, enter a negative value for the number of steps per revolution. If you push your telescope left or up , but the telescope field-of-view indicator on the sky char moves right or down , the sign is probably wrong.
If you are using SkySafari with SkyWire connected to your iPhone, iPad, or iPad Touch, then SkySafari will use SkyWire rather than Wi-Fi to communicate with your telescope.
If you are using SkySafari for Android, then the first two settings below determine how SkySafari communicates with your telescope - either via Bluetooth or Wi-Fi.
These settings are not present in the iOS version of SkySafari. Connect via Bluetooth - If selected, SkySafari will only attempt to communicate with your telescope using a bluetooth serial adapter.
The adapter must be turned on, physically connected to your telescope's serial port, and paired with your Android device.
Connect via Wi-Fi - If selected, SkySafari will only attempt to communicate with your telescope using a Wi-Fi adapter like SkyFi.
The adapter must be turned on, and physically connected to your telescope's serial port. If you are using Wi-Fi, then the following settings must be correct.
These are only used with Wi-Fi telescope communication. They will be disabled if you are communicating via bluetooth, and ignored if you are using SkyWire with an iOS device.
Auto-Detect SkyFi - Detects your SkyFi unit's IP address automatically, using the name you have configured for your SkyFi. This requires SkyFi firmware version 2.
SkyFi Name - The name of the SkyFi device whose IP address you want SkySafari to automatically detect.
Make sure to enter the same name here as you entered into your SkyFi unit's configuration web page! IP Address - If you do not auto-detect your SkyFi's IP address, you can enter it here manually instead.
If you are using a Wi-Fi device that does not respond to SkyFi auto-detection, you must enter its IP address manually. Your mobile device must be on the same Wi-Fi network as the SkyFi, and must have an IP address on the same subnet.
Check your iOS or Android's Wi-Fi network settings to make sure this is correct. Port Number - The TCP port number to be used for communication with the adapter.
Make sure this is the same TCP port that the telescope adapter or server is listening on. You must be connected to SkyFi's wireless network in order to see this web page.
If you have chosen Celestron WiFi as your telescope type, the Communications Settings section described above will not be present. Instead you will see choices for Setup and Control and for Communication.
The Setup and Control screen will have options that vary depending upon the exact Celestron WiFi scope you are connected to. The Communication screen will allow you to change whether you connect to the WiFi directly or by using access point mode where the WiFi scope has joined your local network.
Set Time and Location - If turned on, SkySafari will send the time and location from your mobile device to the telescope when establishing a connection.
This will overwrite your telescope's previously-set time and location. For some telescopes, this may invalidate your alignment.
For older Meade LX telescopes, this may also cause a delay of up to 15 seconds when connecting. Note: This option is disabled with Celestron WiFi scopes.
The time and location is always sent in this case. Readout Rate - The readout rate is how often SkySafari requests the telescope's position from the mount.
If you set this rate to "4 per second", then SkySafari will request the telescope's position and update it on screen four times every second. If the telescope communication drops often, the rate of position requests may be too high for the telescope to respond properly.
Setting a lower rate of 1 or 2 readouts per second may improve reliability. The best readout rate may require some trial and error to find.
A lower readout rate will update the telescope's position in the sky chart less frequently, and may make SkySafari's telescope controls feel sluggish.
Save Log File - If turned on, SkySafari saves a log of its communication with the telescope on your mobile device. SkySafari creates a new log file every time you connect to the telescope.
The log file records every command that SkySafari sends to the telescope, and every response from the telescope.
The log file name contains the date and time you began the telescope session, for example:. This log file can be emailed to Simulation Curriculum for troubleshooting telescope communication problems.
You can transfer the telescope communication log from your iOS or Android device using iTunes file sharing iOS or SD file card transfer Android. Connect your iPhone or iPad to a computer running iTunes with a USB cable.
Select your iOS device when it appears in iTunes, then find the "Apps" section. Choose SkySafari Plus or Pro from the list of apps.
Android users - the scope communication log is written to a folder named "SkySafari Plus" or "SkySafari Pro" at the top level of your SD card.
Copy this file to your computer with a USB cable, or simply email it to yourself. Use the scope display settings to customize the display of the telescope's field of view in the sky chart.
SkySafari will automatically compute the FOV of your equipment and display it in the sky chart when the telescope is connected.
You can enter your equipment into SkySafari using the Equipment settings. See the Equipment Help for more information. To define a particular field of view, tap its row.
You can also enter a custom FOV in degrees if you don't want to choose any equipment from the list. Please Note: if you choose binoculars or a finder scope, you cannot choose an eyepiece or camera.
Binoculars and Finders have built-in eyepieces with fixed fields of view. You can use any eyepiece or any camera with any telescope, however.
Use the "OK" key to cycle through the selection of switches and knobs. Page Rx Setup FS-l6 Digital Proportional Radio Control System 8 RX Setup 8.
The available protocols are: RF Protocol Receiver AFHDS R9B,R6B,R6C,GR3E,GR3F AFHDS 2A A3, A6,X6, iA4B, iA6, iA6B, iA10, iA10B Switching Between AFHDS 2A and AFHDS: 1.
Page Sensors List Use the "UP" and "DOWN" to choose a channel and press "OK" to enter its failsafe settings. Use the "UP" and "DOWN" to turn the failsafe on or off.
Move the channels control surface to the desired position and hold the "CANCEL" key to confirm and exit. Page Asl Pressure FS-l6 Digital Proportional Radio Control System 8.
When an altitude sensor is connected, change the [Air pressure] setting until the altitude is at 0m. Page System Customization 9.
System Customization The FS-i6X's switches and knobs can be moved to other channels. Or if using receivers with more channels, the system can be expanded with extra switches or knobs.
By default, from left to right, the switches and knobs are channels 5, 6, 7, 8, 9 and On the circuit board each channel is labled, making it easy to find the correct channel.
Follow the cables leading from each connector to identify which switch or knob goes to each channel. Remove the 4 screws located on the back of the system and remove the back cover.
Follow the knobs wire and disconnect it form the board. Page Package Contents FS-l6 Digital Proportional Radio Control System Package Contents Channel 2.
Page Product Specification 11 Product Specification Page Appendix 1 Fcc Statement FS-l6 Digital Proportional Radio Control System Appendix 1 FCC Statement This equipment has been tested and found to comply with the limits for a Class B digital device pursuant to part 15 of theFCC rules.
These limits are designed to provide reasonable protection against harmful interference in a residential installation.
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