Search results for "helio"

Converting from coordinates in longitude l... (1)

• Download

Based on lonlat2xy.pro Converts from Helioprojective-Cartesian Coordinate System to Stonyhurst Heliographic Coordinate SystemBased on lonlat2xy.pro http://hesperia.gsfc.nasa.gov/ssw/gen/idl/solar/lonlat2xy.pro Converts from Helioprojective-Cartesian Coordinate System to Stonyhurst Heliographic Coordinate System

Created: 2011-03-02 | Last updated: 2011-03-02

Credits: Anja Le Blanc

Call VSO web service with HELIO input data (1)

• Download

  date transformation from 2000-10-02T23:00:00 to 20001002230000 HELIO instrument names as in http://helio-dev.i4ds.ch/xsd/instruments.xsd spitt into source and instrument names; if these pair don't exist only first part (source) is tried.

Created: 2010-08-04 | Last updated: 2010-08-04

Credits: Anja Le Blanc

Calculate Sun data from date (2)

• Download

caluculates B0 (radians), position angle and sun radius (arcsec) B0 - heliographic latitude of the centre of disk position angle - of the north end of the axis of rotation, measured +ve if east of the north point of the disk radius - the apparent radus of the Sun in arcsec This is created using the calculations from the IDL routine get_sun.pro

Created: 2011-02-15 | Last updated: 2011-03-02

Credits: Anja Le Blanc

Converting from heliocentric coordinate sy... (1)

• Download

Converting from heliocentric coordinate system with coordinates in arcsec to coordinates in longitude latitude Based on the IDL script xy2lonlat.pro http://hesperia.gsfc.nasa.gov/ssw/gen/idl/solar/xy2lonlat.pro Stonyhurst Heliographic Coordinate System to Helioprojective-Cartesian Coordinate System

Created: 2011-02-18 | Last updated: 2011-02-18

Credits: Anja Le Blanc

Check registry for wrongly registed and un... (2)

• Download

HELIO registry contains a list of tables available in the HEC. The HEC contains a table with available talbes itself. This workflow shows the differences between these two lists.

Created: 2012-07-24 | Last updated: 2012-07-24

Credits: Anja Le Blanc

Finding the origins of Solar Wind events a... (6)

• Download

This gives a comprenhensive overview of high speed solar wind events (CME or CIR) seen at Eart, by obtaining the maximum in-situ measure velocity from the data evaluation service (DES), propagating the even backwards to Earth using the HELIO processing service (HPS) and SHEBA propagation model, and search whether halo CMEs or CHs were observed on that time, and retrieves, besides all the previous information, a context solar wind plot (+/- 1 day) and a URL linking to a context movie for CMEs...

Created: 2012-11-16 | Last updated: 2013-03-21

Credits: David PS

Attributions: CME backwards propagation Co-rotating Interaction Regions backwards propagation HFC Synoptic map from date CDAW CME movie from date Solar Wind properties and plot Back CIR-CME propagation model LASCO_CME_QUERY

Associate hessi flares with active regions (3)

• Download

This workflow is querying the HFC ActiveRegions list and HEC hessi_flare list. It requires a time periode and a search radius arround the centre of an Active Region as inputs It produces two outputs: AnnotatedFeatureTable is a modified VOTable where a field is added with the number of associated hessi flares. CombinedTable is a 2 dimensional list with an VOTable for each Active region and one with an VOTable for all associated flares for that Active Region.

Created: 2011-06-22 | Last updated: 2012-07-10

Credits: Donal Fellows

When do the Fastest type II CME should be ... (2)

• Download

The fastest CME is found from an interval of time, and propagated to Earth, in two steps, first to obtain the Solar wind speed at Earth and then propagated again with a more reasonable CME speed. The output produces Min-Max ETAs for each object in the heliosphere and the plots of the final propagation model. This Workflow was produced as one of the challenges in the HELIO CDAW-IV hosted at TCD

Created: 2012-10-21 | Last updated: 2013-03-20

Credits: David PS Eoincar Gab Baptiste Cecconi Shanem Jbyrne Florian Mayer Natasha A lynnyk

Attributions: LASCO_CME_QUERY LASCO_CME_QUERY MDES simple execution timeToTimeRange Forward CME propagation model (SHEBA) - defined outputs When did the fastest type II CME happened? Goes Flare Check WF 100CME_task1 Extract average Solar wind speed from ACE data

When do the Fastest type II CME should be ... (1)

• Download

The fastest CME is found from an interval of time, and propagated to Earth, in two steps, first to obtain the Solar wind speed at Earth and then propagated again with a more reasonable CME speed. The output produces Min-Max ETAs for each object in the heliosphere and the plots of the final propagation model. This Workflow was produced as one of the challenges in the HELIO CDAW-IV hosted at TCD

Created: 2013-03-21

Credits: Gab Anja Le Blanc David PS

Attributions: When did the fastest type II CME happened?

Retrieve Instruments for event dates (2)

• Download

Queries the HELIO ICS web service and returns a list of instruments available for the time periodes in VOTable format

Created: 2010-05-26

Credits: Anja Le Blanc