eVscope Setup Checklist

Tripod Setup
It is safest and easiest to setup and test your tripod completely before mounting your eVscope.
 * While the tripod is horizontal, release the leg extension clamps, extend the legs to the desired length, and close the clamps. Tip: The lower the telescope, the less susceptible it is to wind and vibration
 * Set the tripod up on firm ground and pull the legs out fully to the widest stance. Wooden decks and other surfaces prone to vibration will interfere with Enhanced Vision. (Note you can increase the angle the legs make with the head, refer to the link below.)
 * Watching the bubble level, adjust leg lengths to level the tripod head. (This is essential for good sky tracking.)
 * Double check that the legs are firmly locked into place and will hold the weight of the telescope by firmly pushing down on the top of the tripod.

Once the tripod is level and stable you can mount the eVscope. The eVscope On/Off button may be rotated to any convenient orientation. Holding the base of the telescope down on the tripod head, alternately tighten the mounting screws until just firm. Check the mounting screw tightness occasionally while the scope is on the tripod, they can work loose. The page EVscope tripod operation and maintenance will give you additional information and helpful advice.

Thermalization
Prior to beginning an observing session with a Unistellar telescope it is best to allow the telescope to acclimate to outdoor temperature.

A telescope that has not acclimated will deliver poor quality images for a variety of reasons. If the telescope is warmer or colder than than the ambient outdoor temperature the primary mirror slightly changes its size during the time that it is acclimating. This prevents the telescope from maintaining a good focus. Further a telescope that is warmer than the outside conditions will have currents of warm rising air that can create turbulence within the telescope's tube which will limit image sharpness.

Typically 15 - 30 minutes is enough time to allow the telescope to fully acclimate to outdoor conditions.

Connecting
(Note: This is a summary. Refer to this page on the Unistellar site for details.)

When ready to observe, long press the eVscope power button. The light will be orange for a few seconds, and then will turn steady red. (Go here to learn the meaning of the various LED colors.) Configure your device per the manufacturers instructions to connect to the eVscope WiFi and then open the Unistellar app. The eVscope WiFi Service Set IDentifier (SSID) will look like "eVscopeX-YYYYYY," where Y stands for the eVscope model and YYYYYY is the eVscope unique identifier, part of the serial number.

You will first see the Catalog screen. Tap the Settings icon (gear). This page contains links to Instrument status, Preferences, Manufacturer information, and app Version number. Once the WiFi link is established the My eVscope page contains important status information, and provides access to many functions. Descriptions of these function may be viewed on the

Orientation
Orientation is an eVscope function that allows the scope to determine what direction it is pointing. Together with the time and location provided by the device, Orientation enables the eVscope to precisely point to any sky location and track that location by compensating for the Earth's rotation. If the scope is not tracking the user will be prompted to start Orientation with a button on the Observe (Telescope) screen. Orientation can also be started from the My eVscope page.

Orientation (formerly called Automatic Field Detection, also called Plate Matching) is best performed with the eVscope pointing 45 degrees above the horizon in any direction. The exact elevation and azimuth of the scope is not critical. With stars visible on the Observe screen in Live View, turn the focus knob until stars are roughly in focus. Once begun, Orientation matches the positions of stars in the field against those in its database. It will then automatically point to another position and do the same. This process continues until it is able to calculate its alignment. A bright sky, haze, poor focus, and obstructions will prevent Orientation from completing.

Refer to the Orientation page for further details about this process, and for tips and tricks.

Focusing
Once Orientation has finished it is time to focus. For best results it is essential to focus the eVscope at the beginning of every session after thermal equilibrium is reached. This process minutely changes the distance between the eVscope mirror and image sensor. Refocusing will be needed during an observing session if the ambient temperature changes significantly. This is due to thermal expansion changing the mirror/sensor distance.

To precisely focus the telescope, use the Catalog to find and center a star of moderate brightness in the field of view. Most stars in the Catalog with common names will be suitable. The telescope's Bahtinov mask is used for focusing. It is separated from the dust cap and placed on the front end of the telescope. The mask will diffract the light of the target star into three lines. The process is to adjust the focus wheel at the bottom of the eVscope tube until the center line and the two diagonal lines intersect at the same point and the center line is centered between the two.

Refer to the Focusing page for details on the focusing process and additional tips and advice.

Collimation
While focus optimizes the distance between the mirror and sensor, collimation ensures the mirror and sensor are exactly in line and the mirror point of focus is centered on the sensor. The mirror is held in place in the center of the eVscope tube by the mirror cell, so the only adjustment necessary is the mirror pointing. This is done by adjusting two screws (vertical and horizontal) at the bottom of the tube next to the focus wheel.

Collimation is performed during eVscope production but adjustment may be necessary due to impacts received during shipment and operation. A collimation check procedure will let you know if adjustments are needed. Collimation should be checked periodically or when star images become distorted.

The Collimation page contains step-by-step procedures and advice.

Sensor Calibration
Sensor Calibration is a procedure used to mitigate inevitable temporary and permanent flaws in the eVscope image sensor by identifying them and subtracting them from images. These sensor flaws are largely dependent on the temperature of the sensor and so may change due to the environment. Sensor Calibration should be performed if bright colored flaws appear on the image, and may be performed periodically to generally improve image quality.

In general the procedure is to place the dust cap firmly on the eVscope tube and tap the Sensor Calibration button on the My eVscope page. The eVscope will scan the sensor for bright cells to eliminate from subsequent images. The process takes about two minutes, and does not result in a saved image. The Unistellar Sensor Calibration page provides details on when and how to perform this procedure.