Yohkoh-SXT Campaign Catalog

Yohkoh-SXT Campaign Catalog

1996 - 1999

Title SERTS Rocket Underflight
Begin Date 1999/06/24
End Date 1999/06/24
JOP Number ICAL06
Instruments SXT; SERTS (rocket); TRACE; CDS; SUMER; CELIAS; EIT; Big Bear (GBO); Meudon (GBO)
Campaign Leader Roger Thomas; Barbara Thompson; Jeff Brosius
Purpose DEM observations, EUV calibration
Comments We have selected X = -450 arcsec, Y = +300 arcsec as the center of the 4 arcmin by 4 arcmin CDS field of view for the SERTS flight on June 24. The SERTS roll angle will be 90 degrees, i.e., the slit will be perpendicular to the solar rotation axis. SERTS spectra and spectroheliograms will be obtained at three different, parallel pointings, each separated by 90 arcsec. (Thus the maximum separation between parallel slit pointings will be 3 arcmin.) Ideally, all three slit positions will lie within the CDS, EIT, TRACE, and SXT fields of view. During SERTS launch, SSR will be in record for CDS, 16:15-17:55 UT. One final note about the SERTS pointing for June 24, in case it was not clear from the earlier message: the three SERTS pointing positions will be offset from one another by 90 arcsec in the North-South direction, i.e., perpendicular to our East-West slit orientation. Thus the horizontal slit will twice undergo a 90 arcsec vertical translation during the flight. The center of the 4 arcmin by 4 arcmin CDS field of view remains X = -450 arcsec, Y = +300 arcsec, which corresponds to about 20 degrees North and 30 degrees East.

Title 3-D Structure of Flaring Active Regions
Begin Date 1999/06/15
End Date 1999/06/28
JOP Number JOP098
Instruments SXT; CDS; EIT; MDI; TRACE; OVRO (GBO); Big Bear (GBO); Mees (GBO); Siberian Solar Radio Telescope (GBO); Kitt Peak (GBO); MSFC (GBO); Meudon (GBO); Alfred University (GBO); RATAN 600 Radiotelescope (GBO); Nobeyama (GBO); Mauna Loa (GBO); Nancay (GBO); Kharkov Astronomical Observatory (GBO); Crimean Astrophysical Observatory (GBO); Mitaka (GBO); Oporto Radiospectrograph (GBO); Hiraiso (GBO); Trieste Astronomical Observatory (GBO); IZMIRAN (GBO); San Fernando Observatory (GBO); PHOENIX (GBO); Hida Solar Observatory (GBO); Ondrejov Observatory (GBO); VLA (GBO); Sac Peak (GBO); Brazilian Solar Spectroscope (GBO); Kanzelhoehe (GBO)
Campaign Leader Neale Ranns; Dale E. Gary; Richard Canfield
Purpose To obtain multi-wavelength observations before, during and after solar flares over a wide range of temperatures and heights in the solar atmosphere, for the purpose of building a three-dimensional, topological framework for interpreting HESSI data when they become available, and to bring forth questions that joint studies with HESSI should try to answer;
Comments First Max Millennium Campaign: dry-run for HESSI

Title Active Region Streamer Study
Begin Date 1999/06/07
End Date 1999/06/09
JOP Number Campaign
Instruments SXT; CDS; SUMER; UVCS; TRACE
Campaign Leader Jun Lin
Purpose To study the structure and plasma parameters of bright streamers
Comments

Title Dynamics and Structure of Large Sunspots
Begin Date 1999/06/06
End Date 1999/06/22
JOP Number JOP108
Instruments SXT; CDS; SUMER; CELIAS; EIT; TRACE; SERTS (rocket)
Campaign Leader Brian Handy; Jake Wolfson; Charles Kankelborg
Purpose To obtain a comprehensive set of high resolution images in a large sunspot to study small scale photospheric structures and their effect on, or interaction with, chromospheric oscillations and coronal loops originating from the sunspot.
Comments

Title Transition Region Moss
Begin Date 1999/05/16
End Date 1999/06/05
JOP Number JOP103
Instruments SXT; CDS; MDI; TRACE; SVST (GBO); La Palma (GBO)
Campaign Leader Bart De Pontieu
Purpose The main scientific goals of this JOP are fivefold: one, to investigate temporal variability of the bright moss elements to determine the relative importance of intrinsic changes in brightness and obscuration by chromospheric jets; two, to establish the relationship of moss dynamics to that of underlying magnetic flux elements; three, to investigate how moss relates to cooler transition region structures, e.g. C~IV; four, to study the relationship of changes in emission in hot coronal loops to moss emission; five, to further refine DEM and density measurements, and their temporal variability, for constraint of model parameters.
Comments

Title VAULT Rocket Support
Begin Date 1999/05/07
End Date 1999/05/07
JOP Number Campaign
Instruments SXT; VAULT (Rocket); ; VLA (GBO); Big Bear (GBO); LASCO; EIT; TRACE
Campaign Leader Angelos Vourlidas
Purpose
Comments VAULT (Very High Resolution Advanced Ultraviolet Telescope)

Title X-ray Jets from Limb Active Regions
Begin Date 1999/05/03
End Date 1999/05/15
JOP Number JOP104
Instruments SXT; CDS; SUMER; TRACE
Campaign Leader Davina Innes
Purpose
Comments

Title Active Region 8518 Study
Begin Date 1999/04/19
End Date 1999/04/29
JOP Number Campaign
Instruments SXT; TRACE; Big Bear (GBO); Yohkoh ; Mees (GBO)
Campaign Leader Nariaki Nitta; Carsten Denker; Barry LaBonte
Purpose
Comments

Title Active Region Loop Study
Begin Date 1999/02/24
End Date 1999/02/24
JOP Number Campaign
Instruments SXT; TRACE; MDI
Campaign Leader Harry Warren
Purpose
Comments

Title Active Region Study with Sac Peak
Begin Date 1999/02/04
End Date 1999/02/15
JOP Number Campaign
Instruments SXT; TRACE; Sac Peak (GBO); Big Bear (GBO)
Campaign Leader Richard Shine
Purpose
Comments

Title JOP012 / JOP017
Begin Date 1998/09/04
End Date 1998/09/13
JOP Number JOP012
Instruments SXT; TRACE; Tenerife (GBO); Themis (GBO); La Palma (GBO)
Campaign Leader Bridgitte Schmieder
Purpose
Comments

Title WSM2 JOPs
Begin Date 1998/08/12
End Date 1998/08/25
JOP Number JOP081,84,35
Instruments SXT; TRACE; Kitt Peak (GBO); Sac Peak (GBO); Mees (GBO)
Campaign Leader Sarah Gibson; David Alexander; Vincenzo Andretta
Purpose Due to the unfortunate loss of communications with SOHO, the Second Whole Sun Month Campaign was reduced to a Whole Sun Fortnight (WSF) Campaign. Detailed magnetic field observations (JOP 81) went on much as originally planned. Each day there was coordinated observations between 1400 and 2400 UT in order to take advantage of the time of greatest overlap of magnetic field observations. Depending on solar conditions, each day a different "Target of the Day" (TOD) was chosen from among the following: Active regions (JOP 84) Coronal holes Filament channel (connected to decaying active region) As well as the TOD observations between 1400 and 2400 UT, observations that did not temporally overlap the magnetic field observations (NOO for non-overlap observations) were made for all three targets during the WSF period. Coordinated IPS observations were made throughout the originally scheduled WSM2 period (August 1-28).
Comments

Title Flares in Emerging Flux Regions
Begin Date 1998/07/29
End Date 1998/08/05
JOP Number Campaign
Instruments SXT; Hida (GBO); Hiraiso (GBO); TRACE; Mitaka VMGs (GBO); Huarou VMGs (GBO)
Campaign Leader Hiroki Kurokawa
Purpose
Comments kurokawa@kusastro.kyoto-u.ac.jp

Title High Cadence Activity Studies and the Heating of Coronal Loops
Begin Date 1998/06/14
End Date 1998/06/17
JOP Number JOP083
Instruments SXT; CDS; TRACE; EIT; MDI
Campaign Leader Robert Walsh
Purpose To investigate rapid time variation (down to the order of seconds) within a target coronal loop system and relate these dynamical changes to theoretical models for various coronal loop heating mechanisms.
Comments

Title Magnetic Flux Disappearance in Cancelling Bipoles
Begin Date 1998/06/12
End Date 1998/06/30
JOP Number JOP082
Instruments SXT; CDS; EIT; MDI; YohKoh-; Kitt Peak (GBO); TRACE; Mauna Loa (GBO); Big Bear (GBO); SOONSPOT (GBO)
Campaign Leader Karen Harvey
Purpose
Comments

Title High Time Resolution Imaging
Begin Date 1998/05/13
End Date 1998/05/13
JOP Number JOP080
Instruments SXT: D.McKenzie; EIT:D.Berghmans; MDI:C.Deforest; TRACE:C.Kankelborg; CDS:A.Fludra; SUMER:K.Muglach; Sac Peak(GBO):B.lites; La Palma(GBO):R.Rutten
Campaign Leader Frederic Clette; David Berghmans
Purpose Micro-variability in active region loops at a temperature of 10^6 K with the highest temporal resolution and good spatal coverage (emphasis on imaging instruments) (15 s)
Comments 1 hour duration (17:00-18:00), Submode 5, Target: Active Region

Title Filament Study
Begin Date 1998/05/08
End Date 1998/05/10
JOP Number Campaign
Instruments SXT; TRACE; CDS; MDI; EIT
Campaign Leader Charles Kankelborg (TRACE)
Purpose Filament morphology and evolution in EUV and UV wavelengths. First day (May 9) concentrated on a single FOV, second day interleaved images from several pointings.
Comments May 9 multiwavelength, single FOV May 10 multiwavelength, mosaic of several FOV

Title Study of the Process of Magnetic Flux Dissappearance in Canceling Bipoles
Begin Date 1998/05/04
End Date 1998/05/10
JOP Number JOP082
Instruments SXT; CDS; MDI; TRACE; Kitt Peak (GBO); Big Bear (GBO)
Campaign Leader Karen Harvey; Karel Schrijver
Purpose
Comments

Title St. Andrews Loop Studies
Begin Date 1998/05/02
End Date 1998/05/15
JOP Number JOP059
Instruments SXT; CDS; EIT; MDI
Campaign Leader Robert Walsh
Purpose To obtain temperature, density and magnetic field structure and to investigate high cadence temporal variations within the target coronal loop system
Comments

Title VLA Radio Observations of CMEs
Begin Date 1998/02/21
End Date 1998/02/28
JOP Number Campaign
Instruments SXT; EIT; LASCO; VLA (GBO); Nobeyama (GBO)
Campaign Leader Nat Gopalswamy
Purpose To study thermal and nonthermal signatures of coronal mass ejections (CMEs) using the new metric frequency at 75 MHz. Combination of radio, optical, X-ray and EUV data will be employed to study the CME substructures (frontal arcade, cavity, prominence core) and arcade formation.
Comments Feb 21, 1998 15:05:08 - 23:05:08 UT Feb 23, 1998 14:57:16 - 22:57:16 UT Feb 24, 1998 15:23:15 - 23:23:15 UT Feb 28, 1998 14:37:37 - 22:37:37 UT The New 75 MHz system at the VLA was used for this campaign, in addition to the standard frequencies.

Title Flight of XUV Doppler Telescope aboard ISAS sounding rocket
Begin Date 1998/01/31
End Date 1998/01/31
JOP Number Campaign
Instruments SXT; CDS; EIT; MDI; UVCS; LASCO; Rocketborne XUV Doppler Telescope
Campaign Leader Joe Gurman; Hirohisa Hara (XUV and SXT)
Purpose Provide SOHO imagery, &c. as context for first flight of XDT
Comments Web page set up; no further joint analysis as yet

Title Filaments and Their Environments
Begin Date 1998/01/20
End Date 1998/01/26
JOP Number JOP074
Instruments SXT; VLA (GBO); Nobeyama (GBO); EIT; CDS; MDI; LASCO; Siberan Radio Telescope (GBO); Helio Research (GBO)
Campaign Leader Nat Gopalswamy
Purpose To answer several related questions such as the temperature structure of the filaments, relationship of the prominence cavity seen in radio X-ray and EUV and the extent of corona affected during an eruption.
Comments Two significant eruptive events on Jan 21 and 25 are being investigated using additional data from WIND/WAVES experiment.

Title Limb Loops Campaign
Begin Date 1997/10/08
End Date 1997/10/09
JOP Number Campaign
Instruments SXT; CDS; Norikura (GBO)
Campaign Leader Barbara Bromage
Purpose
Comments

Title Temporal Evolution of Coronal Loops
Begin Date 1997/10/01
End Date 1997/10/12
JOP Number Campaign
Instruments SXT; EIT; VTT Sac Peak - ASP (GBO); MDI
Campaign Leader Tom Metcalf
Purpose
Comments

Title The Smallest Observable Category of Eruptive Filaments
Begin Date 1997/09/18
End Date 1997/09/24
JOP Number JOP050
Instruments SXT; SUMER; CDS; EIT; MDI; Kitt Peak (GBO); Sac Peak (GBO); Helio Research; Big Bear Solar Observatory (GBO)
Campaign Leader Alan McAllister
Purpose 1) define in physical terms the smallest class of filament eruption events as distinguished from other types of macrospicules, (2) understand the processes leading to the formation and eruption of these filaments. (3) investigate their role in the transport of mass, magnetic flux, and energy up into the solar corona, including interactions with large-scale overlying coronal structure.
Comments Data sets were obtained on all 7 days with the SOHO instruments and on 3-4 days for the various GBO sites. 10s of events have been identified from the GBO data and are being used to index the other data sets.

Title Bright Point Campaign
Begin Date 1997/09/08
End Date 1997/09/12
JOP Number Campaign
Instruments SXT; CDS; MDI; EIT; NSO/Kitt Peak (GBO)
Campaign Leader Andrzej Fludra; Lee McDonald (ISAS)
Purpose
Comments 15:00 - 23:00 UT daily, KPNO supplying He I 10830

Title Bright Point Study
Begin Date 1997/07/31
End Date 1997/08/05
JOP Number JOP023
Instruments SXT; CDS; EIT; MDI
Campaign Leader Andrzej Fludra
Purpose To determine the spatial and temporal correspondence between XBPs and the evolution of the magnetic field and structures observed in the chromosphere and corona.
Comments

Title Active Region Diagnostics
Begin Date 1997/07/08
End Date 1997/08/10
JOP Number Campaign
Instruments SXT; CDS; EIT; SUMER
Campaign Leader Helen Mason
Purpose
Comments

Title Multi-Loop Modelling of Active Regions
Begin Date 1997/07/03
End Date 1997/07/06
JOP Number Campaign
Instruments SXT; CDS; EIT; MDI; VLA (GBO)
Campaign Leader Markus Aschwanden
Purpose Stereoscopic reconstruction of active region loops observed at different datys
Comments 17:00 - 01:00 UT

Title X-ray Jets in Coronal Holes
Begin Date 1997/06/30
End Date 1997/07/03
JOP Number JOP057
Instruments SXT; CDS
Campaign Leader Hirohiso Hara
Purpose
Comments 20-22 UT

Title The Smallest Observable Category of Eruptive Filaments
Begin Date 1997/06/09
End Date 1997/06/15
JOP Number JOP050
Instruments SXT; SUMER; CDS; EIT; MDI; NSO/Kitt Peak (GBO); VTT Sac Peak (GBO); Helio Research (GBO)
Campaign Leader Alan McAllister
Purpose Objectives: (1) define in physical terms the smallest class of filament eruption events as distinguished from other types of macrospicules. (2) understand the processes leading to the formation and eruption of these filaments. (3) investigate their role in the transport of mass, magnetic flux, and energy up into the solar corona, including interactions with large-scale overlying coronal structure.
Comments Kitt Peak Filtergraph, VTT Sac Peak/ UBF & ASP,

Title Interplanetary Scintillation Over Limb Structures
Begin Date 1997/06/07
End Date 1997/06/16
JOP Number Campaign
Instruments SXT; CDS; EIT; LASCO; UVCS; EISCAT (GBO)
Campaign Leader Andy Breen
Purpose
Comments 07:15-09:15 UT

Title UV and X-ray Jets_4
Begin Date 1997/05/26
End Date 1997/06/05
JOP Number JOP033
Instruments SXT; CDS; SUMER; EIT; Pic-du-Midi (GBO)
Campaign Leader Brigitte Schmieder
Purpose Multi-instrument high res, high cadence observations of jets, to investigate the possible connection between UV Transition region jets and SXR coronal jets, to determine the physical and plasma properties of jets and to look for evidence of reconnection as the jet driver.
Comments

Title Structure and Variability of Loops
Begin Date 1997/04/03
End Date 1997/04/11
JOP Number JOP059
Instruments SXT; CDS; EIT; MDI
Campaign Leader Robert Walsh; Jack Ireland; Andrzej Fludra
Purpose To obtain temperature, density and magnetic field structure and to investigate high cadence temporal variations within the target coronal loop system.
Comments

Title Diagnostics of Limb Coronal Loops
Begin Date 1997/03/05
End Date 1997/03/10
JOP Number Campaign
Instruments SXT; CDS; EIT; VTT Sac Peak (GBO)
Campaign Leader Andrzej Fludra
Purpose
Comments 16 - 20 UT

Title Filling Factor Studies
Begin Date 1997/02/28
End Date 1997/03/05
JOP Number Campaign
Instruments SXT; CDS
Campaign Leader Sarah Matthews
Purpose To study the fillling factors of coronal loops by using CDS to to compare density measurements made from line ratios and emission measure methods. SXT is used to study the hotter emission; density can only be found from EM method in this case. High time resolution not important.
Comments

Title Filament Movies
Begin Date 1997/02/17
End Date 1997/02/18
JOP Number JOP009
Instruments SXT: Hudson; CDS:Thompson; SUMER:Jordan
Campaign Leader Andrzej Fludra
Purpose To understand the structure of prominences from the standpoint of the physics involved in the energy and force balance, processes that make them form, endure and disappear.
Comments Yohkoh partipates on Feb 18 after 19 UT. Only CDS observes on 17.

Title Off-the-limb Temperature and Density Study of an Active Region
Begin Date 1997/01/18
End Date 1997/01/24
JOP Number Campaign
Instruments SXT; VTT Sac Peak (GBO); CDS
Campaign Leader Paal Brekke
Purpose
Comments CONTRIBUTORS: H.E. Mason, P.R. Young, M.J. Penn, J. Kuhn, P. Brekke, H. Hudson Time requested for CDS: 4 hours per day for 4 days

Title Observations of Polar Jetlets
Begin Date 1996/12/10
End Date 1996/12/17
JOP Number JOP057
Instruments SXT; CDS; EIT; SUMER; Pic du Midi (GBO); VTT Sac Peak (GBO); Sonora (GBO)
Campaign Leader Ken Dere
Purpose We want to clarify the relationship between (quasi- stationary) polar jet like features seen in EUV (EIT), in W-L (Eclipses), and the SXR jets & jetlets recently analysed using SXT sequences from Yohkoh.
Comments

Title Prominence Diagnostics and Dynamics
Begin Date 1996/11/25
End Date 1996/11/30
JOP Number JOP009
Instruments SXT; SUMER; CDS; EIT; GCT Tenerife (GBO)
Campaign Leader Frederic Paletou
Purpose To understand the structure of prominences from the standpoint of the physics involved in the energy and force balance, processes that make them form, endure and disappear.
Comments GCT: 11/29 is the only day when some good data were acquired. The other times either the target was gone or things didn t work very well. Note that the observations start at 10:48 UT. contact: rmolowny@iac.es

Title Vector Magnetogram AR at 45 Degrees Roll
Begin Date 1996/11/21
End Date 1996/11/22
JOP Number Campaign_1
Instruments SXT; EIT; MDI
Campaign Leader Craig DeForest
Purpose
Comments

Title St. Andrews/RAL LOOPS Campaign
Begin Date 1996/11/12
End Date 1996/11/15
JOP Number Campaign
Instruments SXT; CDS; EIT; MDI
Campaign Leader Jack Ireland; Robert W. Walsh; R. A. Harrison; E. R. Priest
Purpose to look for oscillations in loops and to recreate the 3-d magnetic field structure of those loops
Comments a.k.a. St. Andrews LOOPS campaign basically JOP 59 in its first form

Title UV and X-ray Jets_3
Begin Date 1996/10/31
End Date 1996/11/02
JOP Number JOP033
Instruments SXT; CDS; SUMER; UVCS; EIT; MDI
Campaign Leader Lyndsay Fletcher
Purpose Multi-instrument,high resolution,high cadence observations of UV/SXR jets, with the aims of investigating possible connection between UV transition region jets and SXR coronal jets, of determining jet plasma and physical parameters and of searching for evidence of reconnection as jet driver.
Comments see also #570,572;21-24UT; 2 bright points;pole on 11/02;no SUMER 11/01

Title IACG 3 CME Onset Campaign
Begin Date 1996/10/28
End Date 1996/11/20
JOP Number JOP003
Instruments SXT; CDS; EIT; Big Bear (GBO); UVCS; SUMER; Several ground based.
Campaign Leader Terry Kucera; Viggo Hansteen
Purpose To follow a filament or active region as it rotates onto the limb, monitoring for CME s.
Comments SUMER did not participate week 44.

Title X-ray Bright Points_3
Begin Date 1996/10/27
End Date 1996/11/02
JOP Number Campaign
Instruments SXT; MDI; SUMER; CDS; EIT; Big Bear (GBO); CSUN (GBO); Mauna Loa (GBO); SOONSPOT (GBO); NSO/Kitt Peak (GBO)
Campaign Leader Karen Harvey
Purpose
Comments

Title Loop Filling Factor
Begin Date 1996/10/23
End Date 1996/10/25
JOP Number Campaign
Instruments SXT; CDS; EIT;
Campaign Leader James Klimchuk
Purpose To determine the filling factors of hot (> 1 MK) coronal loops. Such filling factors are important for understanding coronal heating.
Comments

Title UV and X-ray Jets_2
Begin Date 1996/10/22
End Date 1996/10/24
JOP Number JOP033
Instruments SXT; CDS; SUMER; EIT; MDI
Campaign Leader Lyndsay Fletcher
Purpose Multi-instrument,high resolution,high cadence observations of UV/SXR jets, with the aims of investigating the possible connection between UV transition region jets and SXR coronal jets, of determining physical and plasma parameters and of looking for evidence of reconnection as the jet driver.
Comments 18-21UT,21-24UT on 24/10;no CDS on 23/10,small efr observed, SUMER jets. See also #570

Title UV and X-ray Jets
Begin Date 1996/10/14
End Date 1996/10/16
JOP Number JOP033
Instruments SXT; CDS; EIT; MDI
Campaign Leader Lyndsay Fletcher
Purpose Multi-instrument high res, high cadence observations of jets, to investigate the possible connection between UV Transition region jets and SXR coronal jets, to determine the physical and plasma properties of jets and to look for evidence of reconnection as the jet driver.
Comments 20-24UT;CDS TRANREG,NFCTR,TEDE22N;EIT 4x4 1min cadnce;pole 14/10 (small jet/spicule),BPs 15,16/10 15/10 no Yohkoh participation

Title Bright Point Study
Begin Date 1996/09/18
End Date 1996/09/20
JOP Number Campaign
Instruments SXT; Mauna Loa (GBO); SUMER; CDS; LASCO; EIT; Big Bear (GBO); NSO/Kitt Peak (GBO)
Campaign Leader Don Hassler
Purpose
Comments

Title Bright Point Lifetimes
Begin Date 1996/09/18
End Date 1996/09/27
JOP Number Campaign
Instruments SXT; LASCO; EIT
Campaign Leader Don Hassler; Eckart Marsch
Purpose
Comments

Title Filament Studies
Begin Date 1996/09/08
End Date 1996/09/17
JOP Number Campaign
Instruments SXT; VLA (GBO); Nobeyama (GBO); EIT; CDS
Campaign Leader Terry Kucera; Nat Gopalswamy
Purpose To determine the temperature structure of filaments and their environments using multiwavength observations.
Comments CDS participated on the 15th and 17th only. VLA data available only for Sep 17

Title Active Region Study
Begin Date 1996/08/26
End Date 1996/08/31
JOP Number Campaign
Instruments SXT; EIT; SUMER; MDI; CDS
Campaign Leader Joe Gurman
Purpose To track an Active Region as it passes the disk with several experiments
Comments Target: NOAA AR 7986 EIT, SUMER, and CDS did not participate 8/26-27/1996 // EIT_support: Aug_28=overlap_field with campaign #260, Aug_29=no EIT, Aug_30-31=171,284,195,304 30min cadence + synoptic //

Title Equatorial Coronal Hole
Begin Date 1996/08/26
End Date 1996/08/31
JOP Number Campaign
Instruments SXT; CDS; SUMER; EIT; CELIAS/MTOF; MDI
Campaign Leader Joe Gurman
Purpose To study the line-of-sight passage of a coronal hole
Comments EIT_support: Aug_27=195 70sec cadence w/171+304 added, Aug_28=overlaps field of capaign #260, Aug_29=no EIT, Aug_30=synoptic, Aug_31=no EIT

Title The Large Scale Structure of the Solar Minimum Corona
Begin Date 1996/08/10
End Date 1996/09/08
JOP Number JOP044
Instruments SXT; LASCO; CDS; SUMER; UVCS; EIT; MDI; SWAN; Mauna Loa (GBO); NSO/Sac Peak (GBO); NSO/Kitt Peak (GBO)
Campaign Leader Sarah Gibson; Douglas Biesecker
Purpose To understand the large-scale, stable, coronal structure of equatorial helmet streamers and polar coronal holes that can persist for several solar rotations at solar minimum.
Comments This campaign is also known as Whole Sun Month, a month of coordinated synoptic observations. For results see: http://serts.gsfc.nasa.gov:80/whole_sun/

Title SOHO/Yohkoh Limb Active Region Study
Begin Date 1996/08/06
End Date 1996/08/08
JOP Number Campaign
Instruments SXT; CDS; SUMER; EIT
Campaign Leader Bob Bentley
Purpose Multi-wavelength study of AR coronal loops
Comments 6:00 - 9:00 daily // No EIT participation on August 6 and 7, Aug 8 EIT only 2x2 summed synoptic at 7:50 UT

Title Transient Brightenings and Magnetic Field Geometry
Begin Date 1996/07/15
End Date 1996/07/18
JOP Number JOP045
Instruments SXT; CDS; SUMER; EIT; Mees Vectormagnetograph (GBO)
Campaign Leader Dana Longcope ; Barbara Thompson
Purpose To study the relation between transient brightenings and magnetic separatrices
Comments On July 15 only CDS, EIT and SUMER, 11-15 UT // No_run_on_July 16. // All on July 17 15-21 UT. July_18:CDS;SUMER; // EIT_support:195,171_1-2min_cadence

Title The Diffuse Corona
Begin Date 1996/07/08
End Date 1996/07/08
JOP Number JOP027
Instruments SXT; LASCO; MDI; SUMER; UVCS
Campaign Leader Eddie Breeveld
Purpose Clarify the nature of the diffuse corona at and above the limb. Determine whether or not the plasma is contained in magnetically closed structures. Determine the plasma properties as a function of height using CDS, SUMER, UVCS and LASCO.
Comments LASCO C1 only

Title Transient Brightenings
Begin Date 1996/06/06
End Date 1996/06/06
JOP Number Campaign
Instruments SXT; SUMER; CDS; Kitt Peak (GBO); EIT
Campaign Leader George Fisher
Purpose Structure and dynamics of Transient Brightenings and Their Relation to Magnetic Field Geometry.
Comments Bright Active Region observed at disk center from roughly 17:00 to 19:00 UT. ; EIT support: 304 synoptic

Title Prominence Observing Program
Begin Date 1996/06/03
End Date 1996/06/09
JOP Number JOP012
Instruments SXT: Mark Weber and Hugh Hudson; SUMER:Terry Kucera; CDS:Bill Thompson and Terry Kucera; Pic du Midi (GBO):Brigitte Schmieder, Jean-Marie Malherbe, and Tierry Roudier; Izmiran (GBO); Ondrejov (GBO); Wroclaw (GBO); EIT
Campaign Leader Brigitte Schmieder
Purpose To determine T, density and v as a function of time in prominences and surrounding. To check the Siphon model of Poland and Mariska
Comments NOTE: This campaign was carried out jointly with campaign # 6 (JOP017); check that record as well. Daily observations from 08:00 - 13:00 UT It is difficult to forcast the presence of a prominence 24 hours before. Due to that we observed small prominences on June 5 and 6. / EIT: 304 2 min cadence June 4-9 /

Title Quiescent Filament or Polar Crown Filament_3
Begin Date 1996/06/03
End Date 1996/06/09
JOP Number JOP017
Instruments SXT; SUMER; CDS; Pic du Midi (GBO); EIT
Campaign Leader Brigitte Schmieder
Purpose To study the dynamics of the transition region of a filament using Si IV lines or O IV and a chromospheric line to coalign with Halpha filament.
Comments NOTE: This campaign has been carried out jointly with campaign # 3 (JOP012); check that record as well. Daily observations from 06:00 - 08:00 UT A long N/S filament has been followed from June 6-9 (E40to W9). / EIT: 304 2 min cadence on June 4 and 6 /

Title X-ray Bright Points_2
Begin Date 1996/05/27
End Date 1996/05/31
JOP Number JOP023
Instruments SXT: Serge Savy; MDI: Ted Tarbell; CDS: Andzej Fludra; EIT: Dan Moses; SUMER; NSO/Kitt Peak (GBO): Karin Harvey; Mees Solar Observatory (GBO): Dick Canfield; Big Bear (GBO): Hal Zirin; Soonspot (GBO): Kiplinger; HAO/CHIP (GBO): Don Hassler
Campaign Leader Karen Harvey
Purpose To determine the spatial and temporal correspondence between XBPs and the evolution of the magnetic field and structures observed in the chromosphere and corona.
Comments The SOHO part of this international campaign is written up as JOP023 (Fludra). // EIT_support:27-30th=304,171,284,195_equator_to_N.Pole

Title VLA-SOHO coordinated observations
Begin Date 1996/05/23
End Date 1996/05/26
JOP Number Campaign
Instruments SXT; SUMER; CDS; EIT; VLA (GBO); Kitt Peak (GBO); Owens Valley Radio Observatory (GBO)
Campaign Leader Markus Aschwanden
Purpose (1) Sunspot gyroresonance stereoscopy (2)Temperature and density structure of active regions (3)Temperature and density structure of quiet corona
Comments Except 05/25, daily observations over 10 hours (15-01 UT). Because the Sun was absolutely quiet (no sunspots, no active regions), the scientific objective (3) was pursued. // EIT_support:synoptic_only_25th_and_26th

Title Filling Factors of Hot Coronal Loops
Begin Date 1996/05/13
End Date 1996/05/16
JOP Number Campaign
Instruments SXT: Serge Savy and Hugh Hudson CDS:Richard Harrison, Andrzej Fludra; SUMER:Klaus Wilhelm, John Mariska; EIT
Campaign Leader James Klimchuk
Purpose To determine the filling factors of hot (> 1 MK) coronal loops. Such filling factors are important for understanding coronal heating. A secondary objective is to evaluate the meaning of filter ratio temperatures measured by the SXT on Yohkoh, given that the observed plasma is unlikely to be isothermal along the line-of-sight.
Comments An active region complex was observed on the disk and at the limb. The data seem adequate for the filling factor measurements. // EIT_support:synoptic

Title X-ray Bright Points
Begin Date 1996/04/06
End Date 1996/04/15
JOP Number JOP023
Instruments SXT: Serge Savy; MDI: Ted Tarbell; CDS: Andzej Fludra; EIT: Dan Moses; SUMER; NSO/Kitt Peak (GBO): Karin Harvey; Mees Solar Observatory (GBO): Dick Canfield; Big Bear (GBO): Hal Zirin; Soonspot (GBO): Kiplinger; HAO/CHIP (GBO): Don Hassler
Campaign Leader Karen Harvey
Purpose To determine the spatial and temporal correspondence between XBPs and the evolution of the magnetic field and structures observed in the chromosphere and corona. KH
Comments The SOHO part of the world-wide campaign is written up as JOP023 (Fludra). SOHO experiments participated on April 8 - 15 // EIT_support:April_6-12,15_@171,195,304,284