Actions: esis-mission/esis
Actions
55 workflow runs
55 workflow runs
esis.data.synth.scene_aia(), a function to download AIA imagery and convert it into a synthetic scene.
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#55:
Pull request #60
closed
by
roytsmart
esis.flights.f2.optics.design(), which represents the current ESIS-II optical design.
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#52:
Pull request #57
closed
by
roytsmart
esis.flights.f2.optics.design_guess() a starting point for optimizing the ESIS-II optical design.
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#51:
Pull request #56
closed
by
roytsmart
esis.flights.f1.optics.design_full() to return exact scalars if num_distribution==0.
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#48:
Pull request #52
closed
by
roytsmart
esis.data.Level_1.from_level_0() to flip the short axis of the CCD to match actual observations.
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#46:
Pull request #51
closed
by
roytsmart
esis.flights.f1.data.level_1() function to load the 2019 Level-1 dataset.
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#44:
Pull request #44
closed
by
roytsmart
esis.flights.f1.optics.as_built() model of the optical system.
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#42:
Pull request #46
closed
by
roytsmart
animate() and to_jshtml() methods to the esis.data.Level_0 class.
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#40:
Pull request #43
closed
by
roytsmart
esis.data.Level_0.dark property to compute the master dark.
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#39:
Pull request #42
closed
by
roytsmart
esis.data.Level_0.despiked property to remove cosmic ray spikes.
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#38:
Pull request #41
closed
by
roytsmart
esis.data.Level_0.darks property.
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#37:
Pull request #40
closed
by
roytsmart
esis.data.Level_0.lights property.
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#36:
Pull request #39
closed
by
roytsmart
esis.data.Level_0.time_mission_start property.
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#32:
Pull request #35
closed
by
roytsmart
esis.flights.f1.data.level_0 function.
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#31:
Pull request #34
closed
by
roytsmart