The value has to be the effective focal length considering all correctors and optical elements that could shift the overall focal length Go to Options->Equipment->Telescope section and set the focal length of your telescope in millimeters. This allows skipping the star alignment process that is typically done during a mount's start-up process.įor a precise centering with a given error margin use the "Repeat until error Equipment->Camera section, the pixel size needs to be entered in micrometers. slew your mount to the location where it was supposed to be in the first place. The former will synchronize your mount's notion of its pointing position to the position that the plate solver has determined is it pointed. To apply the plate solving results to your mount, you need to enable the Sync option and, if desired, the Reslew To Target option in the Plate Solving panel. In the event that both the Primary and Blind plate solving applications fail to produce a result, please verify that your image is in focus and, if necessary, increase the exposure time or change the filter type to allow more stars to be adequately exposed. Thus, the Blind Solver acts as a back up method.īefore being able to plate solve N.I.N.A., any setup that the primary and blind solvers require must be done in accordance with their respective instructions. Where one fails to solve a given image, another might succeed.
#ASTROMETRY ONLINE SOFTWARE#
The reason for this is that while most plate solving software is quite good, none are infallible. will prompt if the Blind Solver should be used to solve the image.
There clicking on the play button a new image will be captured and solved based on the given parameters.
#ASTROMETRY ONLINE MANUAL#
To manual trigger plate solve of an image you need to use the Plate Solving tool in the image panel. This includes the focal length of the telescope itself and any focal length-affecting devices such as reducers, telecompressors, or barlows. will usually be able to detect the sensor's pixel size, but the user will need to inform the software of the effective focal length of the optical path.
The two important settings are the camera's sensor pixel size and the focal length of the telescope. Plate solving requires that your camera and telescope settings are correct.
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