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1) GONG Solar Data from BBSO maxmize
Resource ID:spase://VSPO/NumericalData/Ground/BBSO/GONG/PT86400S
Start:2001-03-14 00:00:00 Observatory:BBSO Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at BBSO Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Big Bear Solar Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

2) GONG Solar Data from Cerro Tololo maxmize
Resource ID:spase://VSPO/NumericalData/Ground/CTIO/GONG/PT86400S
Start:2001-04-20 00:00:00 Observatory:CTIO Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at CTIO Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Cerro Tololo Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

3) GONG Solar Data from Learmonth maxmize
Resource ID:spase://VSPO/NumericalData/Ground/Learmonth/GONG/PT86400S
Start:2001-04-30 00:00:00 Observatory:Learmonth Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at Learmonth Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Learmonth Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

4) Mauna Loa Solar Observatory ACOS/CHIP LOS_Velocity Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/CHIP/LOS-Velocity.Images
Start:1996-04-20 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar line-of-sight velocity images (dopplergrams) and movies from the Chromospheric Helium Imaging Photometer (CHIP, 1083.0 nm) of the Advanced Coronal Observing System (ACOS). As of early 2005, VSO used 'chp' rather than 'CHIP'.

5) Mauna Loa Solar Observatory ACOS/CHIP Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/CHIP/Solar.Images
Start:1996-04-20 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar images and movies from the Chromospheric Helium Imaging Photometer (CHIP, 1083.0 nm) of the Advanced Coronal Observing System (ACOS). As of early 2005, VSO used 'chp' rather than 'CHIP'.

6) Mauna Loa Solar Observatory ACOS/MK4 Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/MK4/Solar.Images
Start:1998-10-01 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar coronal images and movies in white light polarization brightness from the Mark-IV (Mk4) instrument of the Advanced Coronal Observing System (ACOS)

7) Mauna Loa Solar Observatory PICS and DPM Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/PICS-DPM/Solar.Images
Start:1994-02-02 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) H-alpha solar disk and limb images and movies from the Polarimeter for Inner Coronal Studies (PICS) and the Digital Prominence Monitor (DPM) that PICS replaced in September, 1997. PICS is part of the Advanced Coronal Observing System (ACOS). As of early 2005, VSO used 'dpm' for both DPM and PICS.

8) Solar Imagery from Mauna Loa Solar Observatory at HAO maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/Solar.Images
Start:1980-01-01 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar images and movies from the Advanced Coronal Observing System (ACOS), the Experiment for Coordinated Helioseismic Observations (ECHO) and the Precision Solar Photometric Telescope (PSPT). ACOS includes the Chromospheric Helium Imaging Photometer (CHIP, 1083.0 nm), H-alpha prominence and solar disk monitor (PICS, 656.2 nm), and the Mk4 K-coronameter (sees white light K-corona from 1.12 to 2.79 solar radii). ECHO observes oscillations in solar surface radial velocities. PSPT observes the solar disk in three bandpasses: 605-610 nm (red), 408-412 nm (blue) and 393 nm (Ca II K). Some MLSO data contribute to the GONG program.

9) GONG Solar Data from MLSO maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/GONG/PT86400S
Start:2001-06-16 00:00:00 Observatory:MLSO Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at MLSO Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Mauna Loa Solar Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

10) GONG Solar Data from El Teide maxmize
Resource ID:spase://VSPO/NumericalData/Ground/TEIDE/GONG/PT86400S
Start:2001-07-30 00:00:00 Observatory:TEIDE Observatory Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at TEIDE Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from El Teide Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

11) GONG Solar Data from Udaipur maxmize
Resource ID:spase://VSPO/NumericalData/Ground/Udaipur/GONG/PT86400S
Start:2001-10-25 00:00:00 Observatory:Udaipur Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at Udaipur Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Udaipur Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

12) Australian Space Weather Services Learmonth Observatory Spectrograms maxmize
Resource ID:spase://VWO/DisplayData/Learmonth/DS.GIF.PT12H
Start:2000-06-16 05:00:00 Observatory:Learmonth Cadence:
Stop:2016-09-14 08:00:14 Instrument:Learmonth Solar Radiospectrograph Resource:DisplayData
Culgoora and Learmonth Observatories dynamic spectrogram plots display frequency in MHz on the vertical axis and time in UT on the horizontal axis. The time span for each plot varies, generally spanning local day time hours with time resolution of 3 seconds. The frequency range is 18 - 1800 MHz for Culgoora spectrogams and 25 - 180 MHz for Learmonth spectrograms. The intensity values are color coded and are expressed as relative logarithmic units (0 to 255). The Culgoora spectrograms consist of 4 frequency bands: 18-57, 57-180, 180-570 570 -1800 MHz and Learmonth has 2 bands: 25-75, 75-180 MHz. The two Learmonth bands are each divided into 400 frequency steps. Culgoora spectrograph data is available since November 1992, Learmonth data since June 2000.

13) Learmonth Magnetometer 1-hr Data in ASCII Flat Table Format maxmize
Resource ID:spase://VMO/NumericalData/WDC/Learmonth/Magnetometer/PT1H/ASCII_FORMAT
Start:1990-01-01 00:00:00 Observatory:Learmonth Cadence:1 hour
Stop:2010-12-31 23:00:00 Instrument:Learmonth Magnetometer Resource:NumericalData
Learmonth Magnetometer data, 1-hr time resoluion, in ASCII format. Magnetic Field Vector Element List: DHXYZF. Note that the list of magnetic field elements that appear in the data set may change over the course of time. For instance, many stations have shifted from DHZ to the XYZ representation of the magnetic field. The time history listed below summarizes changes in element content. A description of the WDC Data Exchange Format for CADENCE magnetic field data is included at the end of this data product description.

14) Learmonth Magnetometer 1-hr Data in WDC Format maxmize
Resource ID:spase://VMO/NumericalData/WDC/Learmonth/Magnetometer/PT1H/WDC_FORMAT
Start:1990-01-01 00:00:00 Observatory:Learmonth Cadence:1 hour
Stop:2010-12-31 23:00:00 Instrument:Learmonth Magnetometer Resource:NumericalData
Learmonth Magnetometer data, 1-hr time resoluion, in WDC format. Magnetic Field Vector Element List: DHXYZF. Note that the list of magnetic field elements that appear in the data set may change over the course of time. For instance, many stations have shifted from DHZ to the XYZ representation of the magnetic field. The time history listed below summarizes changes in element content. A description of the WDC Data Exchange Format for 1-hr magnetic field data is included at the end of this data product description.

15) Learmonth Magnetometer 1-min Data in ASCII Flat Table Format maxmize
Resource ID:spase://VMO/NumericalData/WDC/Learmonth/Magnetometer/PT1M/ASCII_FORMAT
Start:1993-01-01 00:00:00 Observatory:Learmonth Cadence:1 minute
Stop:2010-12-31 23:59:00 Instrument:Learmonth Magnetometer Resource:NumericalData
Learmonth Magnetometer data, 1-min time resoluion, in ASCII format. Magnetic Field Vector Element List: XYZF. Note that the list of magnetic field elements that appear in the data set may change over the course of time. For instance, many stations have shifted from DHZ to the XYZ representation of the magnetic field. The time history listed below summarizes changes in element content. A description of the WDC Data Exchange Format for CADENCE magnetic field data is included at the end of this data product description.

16) Learmonth Magnetometer 1-min Data in WDC Format maxmize
Resource ID:spase://VMO/NumericalData/WDC/Learmonth/Magnetometer/PT1M/WDC_FORMAT
Start:1993-01-01 00:00:00 Observatory:Learmonth Cadence:1 minute
Stop:2010-12-31 23:59:00 Instrument:Learmonth Magnetometer Resource:NumericalData
Learmonth Magnetometer data, 1-min time resoluion, in WDC format. Magnetic Field Vector Element List: XYZF. Note that the list of magnetic field elements that appear in the data set may change over the course of time. For instance, many stations have shifted from DHZ to the XYZ representation of the magnetic field. The time history listed below summarizes changes in element content. A description of the WDC Data Exchange Format for 1-min magnetic field data is included at the end of this data product description.

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