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* Add missing dDst auxiliary configuration
* Add progress bar for chunks
* PRISM products (#64)
* Temporary workaround allowing loading of the MITx_LP, MITxTEC and PPIxFAC Quality
* Add config for MITx & PPI
* Remove AOB_Quality xarray dimension
* Add PRISM products to docs
Co-authored-by: Martin Paces <[email protected]>
* Add support for external mission MAG products (#65)
* Various fixes needed to support the long-term VOBS data collections.
* Add config for VOBS & .as_xarray(reshape=True) opt
* Fix package installation
* Add model evaluation for data without B_NEC/F vars
* Fix xarray coord attrs
* Try fix shell detection
* Adding VOBS secular variations.
* Minimal changes to work with non-Swarm MAG data.
* Allowing model requests for B_NEC[123] variables
* Support for multiple missions in SwarmRequest.get_times_for_orbits() method.
* Adding GRACE and GRACE-FO spacecrafts.
* Support for CryoSat-2 missions in SwarmRequest.get_times_for_orbits() method.
* Implementing residuals for the CryoSat-2 B_NEC[123] variables.
* Add configuration for Cryosat-2, GRACE, GRACE-FO
* Add multi-mission mag products to docs
Co-authored-by: Martin Paces <[email protected]>
* Update set of VOBS products
* Add access to Swarm positions, MODx_SC
* Update scientific references for collections
* Remove now unused user/password configuration
* Remove nbsphinx dependency from docs
* Adjust get_orbit_number for multi-mission data
* Add missing F variable for MAG_GFO
* Bump to version 0.9.0 for release
Co-authored-by: Martin Paces <[email protected]>
The AUX_OBS collections contain ground magnetic observatory data from `INTERMAGNET <https://intermagnet.github.io/data_conditions.html>`_ and `WDC <http://www.wdc.bgs.ac.uk/>`_. Please note that these data are provided under different usage terms than the ESA data, and must be acknowledged accordingly.
Each VOBS product (e.g. Swarm 1-monthly) is split into two collections (e.g. ``SW_OPER_VOBS_1M_2_`` (containing ``B_OB`` & ``B_CF``) and ``SW_OPER_VOBS_1M_2_:SecularVariation`` (containing ``B_SV``)) because of the different temporal sampling points (i.e. differing ``Timestamp``) of these measurements. Data can also be requested for a specific virtual observatory alone (distinguishable by the ``SiteCode`` variable) with special collection names like ``SW_OPER_VOBS_1M_2_:N65W051`` and ``SW_OPER_VOBS_1M_2_:SecularVariation:N65W051``.
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Calibrated magnetic data are also available from external missions: Cryosat-2, GRACE (A+B), GRACE-FO (1+2):
Copy file name to clipboardExpand all lines: docs/config_details.rst
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Configuration Details
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=====================
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.. note::
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Be careful not to accidentally add your credentials to online repositories or containers. You can use the CLI command ``viresclient clear_credentials`` to remove them.
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While it is possible to enter the server URL and access credentials (see :doc:`access_token`) each time a new request object is created,
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.. code-block:: python
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The older HTTP basic access authentication (i.e. username + password) is still available on the DICS staging server and these credentials can also be configured::
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