{
  "HAPI": "3.2",
  "x_description": "This dataset contains L*, the trajectory along which the second adiabadic invariant is conserved. It is calculated using the International Radiation Belt Environment Modeling (IRBEM) documentation (Boscher, D., S. Bourdarie, P. O'Brien, and T. Guild (2012), IRBEM Library, Version 4.4.0). The calculations are based on Roederer '70. The Tsyganenko89 model is used for the calculations. The electron isotropic distribution is assumed. The product is created by Artem Smirnov. See Smirnov et al, 2020, Adiabatic Invariants Calculations for Cluster Mission, in J. Geophys. Res, 125, e2019JA027576, DOI:10.1029/2019JA027576",
  "cadence": "PT60.000000S",
  "parameters": [
    {
      "type": "isotime",
      "units": "UTC",
      "name": "Time_tags",
      "description": "Interval centered time tag",
      "label": "Universal Time",
      "length": 23,
      "fill": null
    },
    {
      "type": "double",
      "name": "Lstar_value",
      "description": "Spacecraft Lstar value",
      "label": "Lstar value",
      "units": null,
      "fill": "-1"
    }
  ],
  "startDate": "2001-01-01T00:00Z",
  "stopDate": "2019-01-01T00:00Z",
  "x_tap_url": "https://csa.esac.esa.int/csa-sl-tap/data?retrieval_type=HEADER&DATASET_ID=C1_CP_AUX_LSTAR&FORCEPACK=false",
  "sampleStartDate": "2018-11-01T00:00Z",
  "sampleStopDate": "2018-12-01T00:00Z",
  "x_tap_data_url": "https://csa.esac.esa.int/csa-sl-tap/data?RETRIEVAL_TYPE=product&RETRIEVAL_ACCESS=streamed&DATASET_ID=C1_CP_AUX_LSTAR&START_DATE=2018-11-01T00:00:00.000Z&END_DATE=2018-12-01T00:00:00.000Z",
  "status": {
    "code": 1200,
    "message": "OK"
  },
  "x_LastUpdate": "2026-04-12T15:14:00Z"
}