CSES satellite particle flux data¶
Particle flux in the Lshell – pitch reference frame. Lshell will be calculated using the IGRF model for the internal origin field and Tsyganenko model for the external origin field.
References¶
Dataset summary¶
internal_name: |
unitn_flux_cses_timeseries |
publisher: |
Roberto Battiston |
alph_code: |
44 |
id_tmp: |
42 |
short_name: |
CSES Flux |
identifier: |
aspis://unitn/flux_cses_timeseries |
dynamic: |
Static and depending on the length of the input data |
size: |
5MB |
format: |
.mat |
type: |
timeseries |
records_number: |
18129 |
time_start: |
2021-04-12 |
time_stop: |
2021-04-13 |
spatial: |
IONO |
messenger: |
phys.flux |
spectral_min: |
0 |
spectral_max: |
0 |
spectral_units: |
0 |
observable: |
{GCR,ESP,SEP} |
latest update: |
2024-03-28 05:08:17 |
Columns specification¶
progr |
column |
units |
type |
description |
|---|---|---|---|---|
1 |
time |
UTC |
datetime |
datetime (2012-03-01T12:00:00) - time UTC of the data-taking |
2 |
L |
R_E |
float |
R_E Lshell – pitch reference frame |
3 |
En00 |
cm^-2s^-1sr^-1 |
float |
cm^-2s^-1sr^-1 electron and proton flux above 100 KeV |
4 |
En01 |
cm^-2s^-1sr^-1 |
float |
cm^-2s^-1sr^-1 electron and proton flux above 150 KeV |
5 |
En02 |
cm^-2s^-1sr^-1 |
float |
cm^-2s^-1sr^-1 electron and proton flux above 250 KeV |