A plan is a sequence of phases, each with its own capture recipe. The phase table
and the editor for each phase are where you shape exactly what gets captured, and how fast.
The phase set
HelioMaker builds a phase for each stage of the eclipse. For a total eclipse the set runs, in order:
Phase
What it captures
Pre-eclipse
Before first contact; setup and baseline frames.
Partial ingress
C1 → the approach to totality; the shrinking crescent.
Thin crescent · C2
The last sliver before totality (optional; enabled by
Include thin-crescent phase).
Diamond ring · C2
The diamond ring / Baily's beads at second contact.
Totality(or Annularity, or
Central)
The central phase, showing the corona (total), the ring (annular) or the deepest crescent
(partial).
Diamond ring · C3
The diamond ring returning at third contact.
Thin crescent · C3
The first sliver after totality (optional).
Partial egress
C3 → C4; the widening crescent.
Post-eclipse
After fourth contact.
The C3 phases mirror the C2 phases, so what you set going into totality is echoed coming out.
Annular and partial phase sets
Annular and partial eclipses share a simpler five-phase set: Pre-eclipse,
Partial ingress, the central phase, Partial egress and
Post-eclipse. The thin crescent and diamond ring phases belong to a total eclipse only.
The central phase is called Annularity on an annular plan and Central on a
partial one — Central rather than Maximum on purpose, because it is a window minutes wide rather than
the instant of maximum, and naming it after the instant made the two easy to confuse. To widen or narrow that
window, select its row here and use Start before (s): and
End after (s): below.
The phase table
The table lists every phase with its key numbers: Phase, Start,
Duration, Gain, Exposure,
Bracketing, Cycles, Interval,
Shots, Coverage and Guiding. Two narrow
columns flag whether the solar filter is off for the phase and whether a meridian crossing falls inside it. Select
a row to edit that phase below.
Select a row to inspect and edit that phase. The table provides an overview of the complete
exposure and guiding plan.
Preview an HDR bracket and compare it with the recommendations
When you select a bracketed phase, expand Phase summary. It lists every exposure time
in the HDR bracket and reports the full EV span, estimated time per set and total exposure time. This is the
complete capture ladder that results from the selected base exposure, EV step and frame count.
The Tips: panel shows exposure guidance for the selected phase. HelioMaker scales these
recommendations from the plan's measured full solar disk exposure and filter density, and accounts for the
selected eclipse mode. Use the summary and Tips together while changing the recipe so you can see whether the
resulting bracket covers the intended features and still fits the available phase time.
The expanded summary lists every exposure in the selected HDR bracket. Compare the ladder and its
timing with the phase specific Tips while tuning the recipe.
Diamond ring lead and trail times
The C2 and C3 diamond ring phases include Lead time (s): and
Trail time (s):. They extend the selected phase before and after the corresponding
contact, changing how much capture time is devoted to the diamond ring and Baily's beads. The values generated
from Plan preferences... should normally be used unchanged. Experienced eclipse imagers
can adjust them for a specific capture strategy, but should then review the timeline and rehearse the revised
plan. In Diamond ring (Classical) mode, these phase boundaries also determine the filter change points.
Recipe for each phase
Exposure (ms): and Gain:
The exposure and gain for this phase. HelioMaker initially derives them from the measured filtered full
solar disk exposure, the reference camera gain, the effective ND rating of the complete filter stack and
Fred Espenak's eclipse exposure
recommendations. Keeping the same gain for every phase is recommended; make a phase specific gain change
only when physical camera testing supports it.
Bracketing: (EV/step × count)
HDR bracketing specifies how many exposures occur in each cycle and how many EV separate them. Deeper brackets around C2/C3 capture the
huge dynamic range of the inner corona and prominences.
Repeat (cycles):
How many times the recipe repeats within the phase. Max fills the phase's time slot
with as many cycles as fit.
Interval (s):
The time from the start of one cycle to the start of the next, which defines the cadence rather than the gap
between cycles. Max speed sets it to the fastest rate the camera can sustain.
Every imaging interval in the plan is shown in seconds, in the phase table and in this
editor, including the estimated time per cycle beside it. Guiding is the one exception: the guide exposure
and guide interval below remain in milliseconds, which is the unit PHD2 itself uses.
Lead time (s): / Trail time (s):
For the diamond ring phases, how far before and after C2 or C3 the selected phase extends. The same controls
adjust the applicable edge of a thin crescent phase. Plan preferences supplies the initial values; use these
controls only for deliberate phase specific tuning.
Start before (s): / End after (s):(annular and partial central phase)
The same pair of controls, renamed for what they do on the central phase of an annular or partial eclipse:
how long before and after its anchor the phase runs. For annularity the anchor is the pair of
inner contacts, so zero means the phase is exactly C2 to C3 and larger values extend it either side. For a
partial eclipse the anchor is maximum itself, and since there are no inner contacts these two
values are what give the phase its length. Partial ingress and egress take whatever is left on each side.
Overrun:
What to do if a cycle is still running when the phase ends: Cancel & switch or
Finish, then switch.
The Imaging panel changes with the selected phase. This example includes Lead time; a diamond ring
phase provides both Lead time and Trail time for experienced timing adjustments.
Tune a measured plan, not a guessed one
First measure the filtered full solar disk with the actual eclipse rig and enter the exposure, gain and
effective total ND rating in Plan preferences. Let HelioMaker derive the phase
set, then use this
editor to tune it. The phase editor locks when automated imaging starts, so exposure and gain changes must be
completed, approved and rehearsed before the run.
Coverage & intervalInterval is the spacing from the start of one cycle to the start of the next. Coverage reflects how
well the phase samples the changing eclipse. For the partials, the Uniform coverage
option (in Plan preferences) spaces shots by how much the crescent has changed
rather than by a fixed clock interval, so you do not oversample the slow parts or undersample the fast ones.
How many cycles will actually fit?
The C2/C3 bracket cadence and the number of cycles that fit in totality depend on your camera's measured overhead and
the capture mode. In Live view mode each short bracket rung is recorded as several frames
to stay honest, so totality writes many runs of short frames; Still mode captures exact
exposures and usually fits more complete sets. Run the System benchmark test so the
minimum intervals and cycle counts here are realistic, and see Capture mode: Still versus
Live.
When you ask for more cycles than fit
Set Repeat (cycles) higher than the phase's time slot allows and the table shows both
numbers, as 31 (50)* — the scheduled count first, what you asked for in brackets.
The plan description says the same thing in words: 50 requested; 31 fit. HelioMaker does not silently
reduce the request, and it does not pretend the extra cycles will happen.
Shots and recorded frames are different numbersShots counts what you asked the camera for: cycles multiplied by the exposures in the
bracket. A three-exposure bracket repeated 45 times is 135 shots. In Live view a short
rung is recorded as a run of several frames, so the number of files on the disk is larger —
that figure is the recorded frame count, and it is used for disk-space estimates rather than presented as your
shot total.
Per phase guiding within the plan limits
PHD2 guiding: in Plan preferences establishes the
overall guiding policy and populates the phase plan. The Guide this phase: option then
lets you enable or disable guiding for an individual phase where the selected physical setup permits it. The
phase panel also provides Exposure (ms): and Interval (ms): for
the guide camera. A per phase choice cannot override a guiding restriction imposed by the contact window or the
selected camera setup.
The plan-wide Guide interval (ms): is copied to every phase when it changes. Its
allowed range is 500 to 6000 ms, with 2000 to 4000 ms recommended as a starting range. Make any
phase-specific interval adjustment here after applying Plan preferences; keep the interval longer than the guide
exposure.
Use the phase controls to refine the guiding policy supplied by Plan preferences. Controls are
unavailable where the current setup requires guiding to pause.
The C2 and C3 contact windows always pause
HelioMaker disables guiding through the thin crescent and diamond ring phases around C2 and C3 in both physical
setups. Near a contact, the detected target changes from a thinning crescent to beads and then the corona.
Continuing to guide can lock onto the wrong feature and move the mount away from the intended position. The
mount continues tracking during this brief pause, which together with totality normally lasts only a few
minutes. As the photospheric limb grows bright enough for reliable detection after C3, HelioMaker resumes
guiding and returns the Sun to its original locked position.
Guiding inside totality requires a separate guide scope
A Shared camera cannot guide during totality because the same camera is capturing the
eclipse. With a Physical guiding camera, guiding inside totality is available only when
PHD2 guiding: is set to Partial phases and totality in Plan
preferences and guiding remains enabled for the totality phase. This requires the separate guide scope to work
without its solar filter during totality. Review Safety and eclipse modes and rehearse
both filter procedures.
Applying plan changes
When you apply changed Plan preferences, HelioMaker asks before deriving the affected phase settings again.
Within the phase editor, use Max to fill the available time with cycles and
Max speed to choose the fastest sustainable interval. Then adjust the phases you care
about most, usually the C2/C3 group.