scene_aia#

esis.data.synth.scene_aia(time_start, time_stop, wavelength_aia, wavelength_new, radiance, width_doppler, axis_time='time', axis_detector_x='detector_x', axis_detector_y='detector_y', axis_velocity='velocity', num_velocity=1, num_std=3, limit=None)[source]#

Create a synthetic solar scene composed of AIA images.

AIA images from channels wavelength_aia over a supplied time range are used to represent estimates of images at wavelength_new. A supplied mean radiance is assigned to each image at wavelength_new and distributed along axis_velocity into num_velocity bins using a Gaussian with standard deviation width_doppler.

Parameters:

time_start (Time) – The start time of the AIA observations.
time_stop (Time) – The stop time of the AIA observations.
wavelength_aia (Quantity | AbstractScalarArray) – The wavelength label of the AIA channel.
wavelength_new (Quantity | AbstractScalarArray) – The rest wavelength of each spectral line in the synthetic scene replacing wavelength_aia. Elements of wavelength_new should correspond to the elements of .
radiance (Quantity | AbstractScalarArray) – The average radiance of each spectral line in the synthetic scene in units of \(\text{erg}\,\text{cm}^{-2}\,\text{sr}^{-1}\,\text{s}^{-1}.\)
width_doppler (Quantity | AbstractScalarArray) – The average standard deviation of each spectral line in the synthetic scene.
axis_time (str) – The logical axis corresponding to changes in time.
axis_detector_x (str) – The logical axis corresponding to changes in detector \(x\)-coordinate.
axis_detector_y (str) – The logical axis corresponding to changes in detector \(y\)-coordinate.
axis_velocity (str) – The logical axis corresponding to changes in line-of-sight velocity.
num_velocity (int) – The number of velocity bins in the synthetic scene.
num_std (float) – The size of the domain for each spectral line in standard deviation units.
limit (None | int) – The maximum number of files to download per wavelength.