Tools and Utilities
Dark Frames
Manual Guide
Auto-Select Star
Calibration Data
PHD2 Server
Drift Alignment
Lock Positions
Equipment Profiles
Simulator Parameters
Dark Frames
Normally, PHD2 saves
dark frames automatically as part of the 'Take Dark' function,
and dark frames can be captured for the various exposure times you
want to use. However, these dark frames are discarded when PHD2
shuts down. If you want to build a permanent library of dark
frames that can be re-used across program executions, you should take
dark exposures for each exposure duration you anticipate using, then
click on a 'Save Dark Frames' under the 'Tools' menu. The
entire set of dark frames will be stored in a single file, in the
location you choose. In a subsequent PHD2 session, you can reload
the dark frames file, and PHD2 will use the appropriate dark frame
based on your exposure duration. You can also choose to have this
done automatically from the 'Camera' tab in Advanced Settings.
Since dark frames primarily help to reduce thermal noise, you might
want to maintain dark sets for different temperature ranges, perhaps
one for winter and another for summer.
Manual Guide

If
you are connecting to a new mount and are encountering calibration
problems, you will probably want to be sure that PHD2's
commands are
actually getting to the mount. Or you may want to nudge the mount or
experiment with manual dithering. In the 'Tools' menu, click on
'Manual
Guide' and
a dialog will appear to let you move the mount at guide speed in any
direction. Each time you press the button, a pulse of the duration
specified in the 'Guide Pulse Duration' field will
be sent. The default value is the 'calibration step-sze' set in
the Advanced Options dialog. If you are debugging calibration
problems, listen to (rather than watch) your mount to determine if the
mount is getting
the commands from PHD2. The idea here is just to figure out if the
mount is responding
to PHD2's
signals. You won't be able to see the mount move (it's moving
at guide speed)
but you may be able to hear it. Other options include watching the
motors themselves or
attaching a laser pointer to your scope and aiming it at something
fairly far away (to amplify your motions). If you have an
adaptive optics device attached, you'll see separate move buttons for
both the AO and the secondary mount.
Dithering
is used primarily with image capture or automation applications,
usually through the PHD2 server interface. However, you can do
manual dithering or experiment with dither settings using the controls
at the bottom of the dialog. The 'dither' amount field at the
left controls the amount the mount will be moved , in units of
pixels. You can scale this amount - i.e. multiply it by a
constant - by using the 'scale' spin control to the right. These
two controls establish a maximum amount of movement that will be used
for dithering - the product of 'scale' X 'dither'. When you click
on the 'Dither' button, PHD2 will move the mount by a random amount
that is less than or equal to the limit you have set, in one of the
north/south/east/west directions. The 'RA Only' checkbox will
constrain the dither adjustments to only east or west. Obviously,
if you are doing a manual dither in this way, you'll want to be sure
your imaging camera is not in the middle of an exposure.
Auto-Select Star
Clicking
on 'Auto-select Star' under the 'Tools' menu, or using the keyboard
shortcut of <Alt>S, tells PHD2 to scan the current guide image
and identify a star suitable for guiding. This operation requires
that 'Looping' is active. The selection process is based on the
shape and brightness of the star but it doesn't consider close
proximity to other stars.Manual Control of Calibration Data
Calibration
data is saved automatically each time a calibration sequence completes
successfully. The use of the calibration data has been described
elsewhere (Using PHD Guiding),
including options for restoring calibration data from an earlier
time or "flipping" it after a meridian flip. You access these
functions using the 'Tools' menu. One other
calibration-related item is also shown there, namely the option to
enter calibration data manually. You should use this only under
very unusual circumstances and only if you're sure you know what you're
doing; but it is available as a matter of completeness. If you
click on the 'Enter calibration data' item, you'll see a dialog box
that allows input of relatively low-level calibration data. This
data might come from a much earlier session, perhaps extracted from the
PHD2 guiding log file.
PHD2 Server
PHD2 supports third-party imaging and automation applications that need to control the guiding process. Stark Labs' Nebulosity program
was the first to do this, but other applications have subsequently been
produced. By using the PHD2 server process, image capture
programs can control dithering between exposures or suspend guide
exposures while the primary imaging camera is downloading data.
To use these capabilities with a compatible application, you
should click on the 'Enable Server' option under the 'Tools'
menu. The server interface has been reworked substantially in
PHD2, and it's now possible for an application to control most aspects
of PHD2's guiding operations. Documentation for the server API is
available on the PHD2 Wiki.
Drift Align
Drift
alignment is a
well-known technique for achieving polar alignment and is considered by
many to be the "gold standard". The Drift Alignment tool is a
"wizard-like" sequence of dialogs that can help you work through the
drift alignment process and get quantifiable results. Once you've
calibrated your guider, click on 'Drift Align' under the 'Tools' menu.
The first Drift Align dialog will appear to help you adjust the
azimuth on your mount. If you are using an ASCOM mount, you'll
have the option of slewing to an area near the celestial equator and
the celestial meridian. If you're not using an ASCOM mount,
you'll need to slew to that location manually. Once the scope is
positioned and you have a suitable star in the field of view, click on
the 'Drift' button to begin collecting data. You'll see the graph
window with a display of star deflections and corrections and, more
importantly, two trendlines. Let the exposures continue until the
declination trendline has stabilized and is no longer jumping around
with each new exposure. At the bottom of the graph window, you'll
see a measurement for the polar alignment error in azimuth. Now
click on the 'Adjust' button to halt guiding, then make a
mechanical adjustment in azimuth. Once done, click on the 'drift'
button again to repeat the measurement. Continue iterating in
this way until you are satisfied with your azimuth accuracy. You
can use the 'notes' field to record which way the drift line moves
depending on how you make the adjustment. For example, you might
note that a counter-clockwise turn of the mount altitude moves the
drift line "up." Since these notes are retained across PHD2
sessions, subsequent drift alignments will probably proceed more
quickly.
Until
you are experience with drift aligning your particular mount, the
'adjustment' part of the process can be a bit tedious. At first,
you'll have to determine how to adjust a knob on the mount to achieve
the desired effect: "how much" and "what direction." To help with
this, the PHD2 drift align
tool supports "bookmarks". These are a handy way to record the
positions of the guide star before and after you've made an adjustment.
Bookmarks are accessed using keyboard shortcuts, as follows:
- b : toggle/show bookmarks
- Shift-b : set a bookark at the current guide star position (the "lock position")
- Ctrl-b : clear all bookmarks
- Ctrl-click somewhere on the image : set a bookmark at that position, or remove the bookmark that's already there
By
setting a bookmark before you make a mount adjustment, you can get a
clear view of how the adjustment has moved the star on the guide frame.
Next,
click on the 'Altitude' button.
Then slew the scope to a position near the celestial equator and
25-30 degrees above the horizon. Click on the 'drift' button to
begin collecting data for the altitude part of the alignment process.
As before, you will iterate between making adjustments and
measuring your alignment until you are satisfied with the result,
keeping notes as you go about how mount adjustments affect the behavior
of the drift line.
If you make substantial adjustments in altitude, you'll need to
go back to the 'azimuth' measurement and repeat that procedure.
If you work through these procedures systematically, you'll
converge on a good polar alignment with a known degree of accuracy.
A good polar alignment will help your guiding performance,
especially in declination.
Lock Positions
PHD2 normally
sets a 'lock position' where the guide star is located at the end of
calibration. Depending on the details of the calibration
sequence, this may not be exactly where the star was located at the
start of calibration - it could be off by a few pixels. If you
are trying to precisely center your target, you may want to use a
'sticky lock position.' You do this by clicking on your guide
star before calibration, then
setting the 'Sticky Lock Position' under the 'Tools' menu. After
calibration is complete, PHD2 will continue to move the mount until the
star is located at the sticky lock position. So you may see
an additional delay after the calibration while PHD2 repositions the
scope at guide speed. The sticky lock position will continue to
be used even as guiding is stopped and subsequently resumed.
Again, this insures a rigorous positioning of the guide star (and
presumably your image target) at the expense of delays needed for PHD2
to reposition the mount.Managing Equipment Profiles
Equipment profiles were introduced in the section on Basic Use
where they are used as part of the 'Connect Equipment' dialog. If
you want to manage multiple profiles, you will probably want to use the
'Manage Profiles' button in the 'Connect Equipment' dialog. Using
the menu items there, you can create a new profile
or edit/rename/delete an existing one. Each profile holds
all the settings that were active at the time the profile was last
used. If you create a new profile, you can import these settings
from either the PHD2 defaults or from an existing profile. To
edit the settings in an existing profile, you first select it in the
equipment profile drop-down list, then click on 'Settings' under the
'Manage Profiles' pull-down. This will take you to the 'Brain'
dialog, where you can make whatever changes you want. Remember
than profiles are automatically updated anytime settings are changed
during a PHD2 session. Finally, you can import and export
profiles for purposes of debugging, backup, or even exchange with other
PHD2 users.
Advanced Settings for the Simulators
The device simulators were introduced in the Basic Use
section as useful tools for you to experiment with PHD2 and become
famliar with its features. Remember that you must choose
'Simulator' as the camera type and 'On-camera' as the mount type in
order to get the benefits of simulation. As you become more
interested in the details of the simulation, you can use the 'Cam
Dialog' button on the main display to adjust the simulation parameters:

You
can adjust simulated mount behaviors for declination backlash, drift
due to polar mis-alignment, and periodic error. You can also
adjust the 'seeing' level, which will create fairly realistic guide
star deflections that look like seeing effects. If you adjust
these parameters one-by-one, you'll see how they affect star
deflections and how the different guide algorithms react to those
movements. Of course, you're dealing with a "nearly perfect" mount in
these scenarios (except for backlash), so the simulation can't be entirely realistic.