Presentation is loading. Please wait.

Presentation is loading. Please wait.

CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G H.-S. Yu, P.P. Hick, A. Buffington University of California at San Diego, LaJolla, California,

Published byErnest Walker Modified over 8 years ago

Similar presentations

Presentation on theme: "CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G H.-S. Yu, P.P. Hick, A. Buffington University of California at San Diego, LaJolla, California,"— Presentation transcript:

1 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G H.-S. Yu, P.P. Hick, A. Buffington University of California at San Diego, LaJolla, California, United States Masayoshi http://smei.ucsd.edu/ http://ips.ucsd.edu/ D. Odstrcil George Mason University, Fairfax, Virginia, United States M. Tokumaru Nagoya University, Japan (Email: bvjackson@ucsd.edu) An Account of Space Weather at Comet 67P/C-G B.V. Jackson University of California at San Diego, LaJolla, California, United States With help from

2 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Data Sets/Analyses: Interplanetary scintillation (IPS) mainly from STELab, Japan, ACE, CELIAS, Wind data near Earth, Rosetta SREM and IES data Heliospheric Tomography: 3-D Heliospheric Tomography (a kinematic model fit to data – a time-dependent heliospheric Earth view from a single location) Speeds and densities from the IPS, vector fields from solar surface magnetic field maps Current Applications: Real time heliospheric views IPS-Driven ENLIL Rosetta data and puzzles; how the solar wind fits in. Future: Better and more precise continuously verifiable analyses? Introduction:

3 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G What Can We Say about the Solar Wind at Comet 67P/C-G and Rosetta?

4 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Densities and Velocities on the Ecliptic Plane Density Velocity

5 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Densities and Velocities on the Earth-Sun Meridian Density Velocity

6 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Velocity at Rosetta Density at Rosetta Density at Earth Velocity at Earth

7 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G How is this Done? Interplanetary Scintillation (IPS) Analysis

8 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G STELab IPS array near Mt. Fuji DATA STELab IPS array systems IPS Heliospheric Analyses (STELab)

9 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G IPS line-of-sight response DATA STELab IPS array systems IPS Heliospheric Analyses (STELab)

10 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G New STELab IPS array in Toyokawa (3,432 m 2 array now operates well – year-round operation began in 2011) Current STELab Toyokawa IPS System

11 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Sample outward motion over time Heliospheric C.A.T. analyses: example line-of-sight distribution for each sky location to form the source surface of the 3D reconstruction. IPS line-of-sight response Jackson, B.V., et al., 2008, Adv. in Geosciences, 21, 339-360. STELab IPS

12 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G IPS C.A.T. Analysis Bastille Day Event 14 July 2000 Jackson, B.V., et al., 2002, Solar Wind 10, 31 IPS Density Remote View

13 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G IPS C.A.T. Analysis Bastille Day Event 14 July 2000 Jackson, B.V., et al., 2002, Solar Wind 10, 31 IPS Density Ecliptic Cut

14 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G IPS C.A.T. Analysis Bastille Day Event 14 July 2000 Jackson, B.V., et al., 2002, Solar Wind 10, 31 IPS Velocity Ecliptic Cut

15 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Zhao, X. P. and Hoeksema, J. T., 1995, J. Geophys. Res., 100 (A1), 19. http://ips.ucsd.edu/ Magnetic Field Extrapolation 1.Inner region: the CSSS model calculates the magnetic field using photospheric measurements and a horizontal current model. 2.Middle region: the CSSS model opens the field lines. In the outer region. 3.Outer region: the UCSD tomography convects the magnetic field along velocity flow lines. Dunn et al., 2005, Solar Physics 227: 339–353. Jackson, B.V., et al., 2012, Adv. in Geosciences, 30, 93-115.

16 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G IPS Forecasts

17 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G UCSD IPS analysis Web Analysis Runs Automatically Using Linux on a P.C. http://ips.ucsd.edu/ UCSD Web pages Real-Time Forecasts Jackson, B.V., et al., 2011, Adv. in Geosciences, 30, 93-115.

18 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Forecast Web Analysis Runs Automatically Using Linux on a P.C. http://ips.ucsd.edu/ One CME just passed 2013/05/14 4-6 UT increase by ~8 Np/cc Jackson, B.V., et al., 2011, Adv. in Geosciences, 30, 93-115. Fit to CELIAS data

19 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G One CME just passed 2013/05/14 4-6 UT increase by ~8 Np/cc Forecast http://ips.ucsd.edu/ Web Analysis Runs Automatically Using Linux on a P.C. One CME just passed 2013/05/14 4-6 UT increase by ~8 Np/cc Jackson, B.V., et al., 2011, Adv. in Geosciences, 30, 93-115. Fit to CELIAS data

20 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Pearson’s r correlation coefficient, day to day forecast verification Correlations (from UCSD forecast) Jackson, B.V., et al., 2010, Solar Phys., 265, 245-256. Jackson, B.V., et al., 2011, Adv. in Geosciences, 30, 93-115. Five day behind “aftcast” One day ahead forecast Velocity Density Velocity Density Velocity matched to ACE, density matched to CELIAS Remote velocity from STELab IPS three-site Remote density from STELab IPS g-level

21 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Web Analysis Runs Automatically Using Linux on a P.C. http://ips.ucsd.edu/ EarthRadial and Tangential Magnetic Field Jackson, B.V., et al., 2012, Adv. in Geosciences, (in press).

22 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Pearson’s r correlation coefficient, day to day forecast verification Correlations (from UCSD forecast) Jackson, B.V., et al., 2011, Adv. in Geosciences, 30, 93-115. Five day behind “aftcast” One day ahead forecast B radial B tangential B radial B tangential RTN coordinates

23 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G The first new data from the on-board Standard Radiation Environment Monitor (SREM) instrument are shown in the attached figure which presents the charged particle count rates observed in two energy channels of SREM: TC3, which is sensitive to protons from roughly 27 MeV energy upward, and TC2 from 49 MeV on. The counts observed give an indication of the Galactic Cosmic Ray (GCR) environment encountered by Rosetta at its then location at 4.4 AU distance from the Sun. These measurements were made during a solar maximum period and are a factor ~2 lower than in February 2011 which was during the previous solar minimum. This is as expected by the variation of the GCR fluxes over the 11-year solar cycle.

24 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G From: Stil@nuim.ie Sent: Tuesday, August 19, 2014 3:32 AM To: bvjackson@ucsd.edu Subject: Space Weather at Comet 67P/C-G Dear Bernie, I am excited to have received from the SREM Team the attached beautiful signature of an SEP at Rosetta recorded in February-March of this year in, as an example, SREM channels TC1, TC2 and TC3 corresponding to >20, >40 and >10 MeV protons. Also SEP Onset at STEREO A & B ~2.5 UT, Earth 25 ~14 UT

25 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G IES Quicklook plots for Aug-Oct indicating observation of solar activity Kathy Mandt, Jim Burch, Ray Goldstein, IES team Oct. 13, 2014

26 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Dates of observations of solar wind activity August 28 solar wind energy increase at ~19:00 September 1 – increased background due to SEP starting at 18:00 September 11 solar wind energy increase at 10:00 September 19 solar wind energy increase at 12:00 September 24 – increased background due to ?SEP? starting at 23:00 October 10 solar wind energy increase at 18:00 October 11 solar wind energy increase at 07:00

27 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Increase in SW energy at ~19:00

28 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Increasing background due to SEP?

29 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G

30 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Increase in SW energy at ~10:00

31 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Increase in SW energy at ~12:00

32 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Increasing background due to SEP?

33 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Increasing background due to SEP?

34 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Increase in SW energy at ~20:00

35 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Increase in SW energy at ~07:00

36 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G From: Mandt, Kathleen Sent: Monday, October 27, 2014 1:08 PM To: Bernard V. Jackson ; Ip Wing-Huen ; Fuselier, Stephen Cc: Burch, Jim ; Goldstein, Ray ; Susan McKenna-Lawlor ; Dusan Odstrcil ; Dave Webb ; Mario Bisi ; Munetoshi Tokumaru ; Sunhak Hong ; Americo Gonzalez ; Julio Cesar Mejia Ambriz Subject: Re: NEWS UPDATE Hi Bernie et al., We have more dates to give you for activity at Rosetta. We saw what appears to be a shock on Oct. 13 at 17:00, another one on Oct. 22 at 16:00 and again on Oct. 25 at 01:00. The data from Oct. 25 seems to have a high background which may indicate more energetic particles in the solar wind. Kathy

37 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Large X1.6 flare N14 E06 beginning September 10, 17:21 UT, and a Halo CME. Density at Rosetta

38 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Velocity at RosettaDensity at Rosetta

39 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Density Velocity Densities and Velocities on the Ecliptic Plane Real time forecast updated ever 6 hours at: Rosetta Earth ftp://cass185.ucsd.edu/data/IPS_Rosetta_Real_Time

40 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G

41 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G a Comprehensive Model Toward that Includes 3D-MHD

42 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Subject: SOHO/LASCO HALO CME 140418ab (Kevin Schenk) UCMEO 93001 40418 1930/ 40418 61325 81742 1771/ 170// 333// 41208 40418 61233 81318 33118 12036 1112/ 99999 (Frontsided) SOHO/LASCO observed two (2) HALO CMEs in close succession April 18, 2014. The events are first seen in C2 at 13:25 UT as a bright loop in progress over the Southwest. The front expands with extensions to a full HALO CME by 13:36 UT. The event continues into the C3 field beginning 13:30 to 17:42 UT leaving the C3 field of view at 30Rsun in the South. April 18 2014 halo CME

43 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G April 18 2014 halo CME IPS Forecast

44 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G IPS-Derived Boundaries for 3D-MHD Models (Yu, H-S., et al., 2012, AIP Conference Proc. 1500, pp. 147-152.)

45 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G UCSD IPS Data Fit Model Ecliptic Cuts Kinematic Model Iterative Data Fit ENLIL 3D-MHD forward modeling from a 21.0 Rs 3D time-dependent IPS tomography boundary Density http://spaceweather.gmu.edu/projects/enlil/ipsbd/density.html

46 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G UCSD IPS Data Fit Model Ecliptic Cuts Kinematic Model Iterative Data Fit ENLIL 3D-MHD forward modeling from a 21.0 Rs 3D time-dependent IPS tomography boundary Density http://spaceweather.gmu.edu/projects/enlil/ipsbd/density.html

47 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G Better than IPS or Cone Model ENLIL?

48 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G SMEI Webpages - http://smei.ucsd.edu SMEI proton density reconstruction for the 27-28 May 2003 halo CME sequence. Reconstructed and ACE L2 in-situ densities are compared over one Carrington rotation. Full SMEI data set, 6-hour cadence, 3º x 3º lat, long 27-28 May 2003 CME event period Jackson, B.V., et al., 2008, J. Geophys Res., 113, A00A15, doi:10.1029/2008JA013224

49 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G All sky view to within 2º (7.5Rs) of the Sun Cut-away and schematic Characteristics Jackson,B.V., et al., 2004, Solar Phys., 225, 177-207. Jackson,B.V., et al., 2010, Solar Phys., 265, 257–275. SMEI heritage ASHI – A Light-weight All Sky Heliospheric Imager

50 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G ASHI tests with a cooled CCD camera Night sky throughput tests Optic before diamond turning Diamond turned optic Optic stray light tests Buffington, A., et al., 2009, Proc. of SPIE, Vol. 7438, 74380O-1-12, doi: 10.1117/12.825362 Jackson, B.V. et al., 2014, Space Weather Workshop, NOAA ASHI – A Light-weight All Sky Heliospheric Imager

51 CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G The IPS analysis is a ground-based technique that can provide low-resolution velocity and density analysis, and forecasts of time-variable heliospheric structure. The present Rosetta data seem to be explained pretty- well by the solar wind analyses -- with questions. Both ENLIL driven with IPS and ENLIL with cone model inputs and WSA inputs work pretty well. In the future higher-resolution autonomous space- based systems are available, resources permitting. Summary:

Download ppt "CASS/UCSD SALE 2014 An Account of Space Weather at Comet 67P/C-G H.-S. Yu, P.P. Hick, A. Buffington University of California at San Diego, LaJolla, California,"

Similar presentations

K. Fujiki, H. Ito, M. Tokumaru Solar-Terrestrial Environment Laboratory (STELab), Nagoya University. SOLAR WIND FORECAST BY USING INTERPLANETARY SCINTILLATION.

K. Fujiki, H. Ito, M. Tokumaru Solar-Terrestrial Environment Laboratory (STELab), Nagoya University. SOLAR WIND FORECAST BY USING INTERPLANETARY SCINTILLATION.
The Johns Hopkins University Applied Physics Laboratory SHINE 2005, July 11-15, 2005 Transient Shocks and Associated Energetic Particle Events Observed.

The Johns Hopkins University Applied Physics Laboratory SHINE 2005, July 11-15, 2005 Transient Shocks and Associated Energetic Particle Events Observed.
H.-S. Yu Center for Astrophysics and Space Sciences, University of California at San Diego, LaJolla, CA, USA 3D-MHD Models Driven by IPS

H.-S. Yu Center for Astrophysics and Space Sciences, University of California at San Diego, LaJolla, CA, USA 3D-MHD Models Driven by IPS
Global Properties of Heliospheric Disturbances Observed by Interplanetary Scintillation M. Tokumaru, M. Kojima, K. Fujiki, and M. Yamashita (Solar-Terrestrial.

Global Properties of Heliospheric Disturbances Observed by Interplanetary Scintillation M. Tokumaru, M. Kojima, K. Fujiki, and M. Yamashita (Solar-Terrestrial.
Inner Source Pickup Ions Pran Mukherjee. Outline Introduction Current theories and work Addition of new velocity components Summary Questions.

Inner Source Pickup Ions Pran Mukherjee. Outline Introduction Current theories and work Addition of new velocity components Summary Questions.
Understanding Magnetic Eruptions on the Sun and their Interplanetary Consequences A Solar and Heliospheric Research grant funded by the DoD MURI program.

Understanding Magnetic Eruptions on the Sun and their Interplanetary Consequences A Solar and Heliospheric Research grant funded by the DoD MURI program.
Understanding Magnetic Eruptions on the Sun and their Interplanetary Consequences A Solar and Heliospheric Research grant funded by the DoD MURI program.

Understanding Magnetic Eruptions on the Sun and their Interplanetary Consequences A Solar and Heliospheric Research grant funded by the DoD MURI program.
February 26, 2007 KIPAC Workshop on Magnetism Modeling/Inferring Coronal And Heliospheric Field From Photospheric Magnetic Field Yang Liu – Stanford University.

February 26, 2007 KIPAC Workshop on Magnetism Modeling/Inferring Coronal And Heliospheric Field From Photospheric Magnetic Field Yang Liu – Stanford University.
Coronal and Heliospheric Modeling of the May 12, 1997 MURI Event MURI Project Review, NASA/GSFC, MD, August 5-6, 2003 Dusan Odstrcil University of Colorado/CIRES.

Coronal and Heliospheric Modeling of the May 12, 1997 MURI Event MURI Project Review, NASA/GSFC, MD, August 5-6, 2003 Dusan Odstrcil University of Colorado/CIRES.
RT Modelling of CMEs Using WSA- ENLIL Cone Model 2014-06-04 1.

RT Modelling of CMEs Using WSA- ENLIL Cone Model
The Sun and the Heliosphere: some basic concepts…

The Sun and the Heliosphere: some basic concepts…
1 C. “Nick” Arge Space Vehicles Directorate/Air Force Research Laboratory SHINE Workshop Aug. 2, 2007 Comparing the Observed and Modeled Global Heliospheric.

1 C. “Nick” Arge Space Vehicles Directorate/Air Force Research Laboratory SHINE Workshop Aug. 2, 2007 Comparing the Observed and Modeled Global Heliospheric.
CASS/UCSD AFOSR 2014 IPS 3D Velocity and Density Analysis B.V. Jackson Center for Astrophysics and Space Sciences, University of California at San Diego,

CASS/UCSD AFOSR 2014 IPS 3D Velocity and Density Analysis B.V. Jackson Center for Astrophysics and Space Sciences, University of California at San Diego,
CASS/UCSD KSSS 2014 3D Analysis of Remote-sensed Heliospheric Data B.V. Jackson, H.-S. Yu, P.P. Hick, A. Buffington University of California at San Diego,

CASS/UCSD KSSS D Analysis of Remote-sensed Heliospheric Data B.V. Jackson, H.-S. Yu, P.P. Hick, A. Buffington University of California at San Diego,
Evolution of the 2012 July 12 CME from the Sun to the Earth: Data- Constrained Three-Dimensional MHD Simulations F. Shen 1, C. Shen 2, J. Zhang 3, P. Hess.

Evolution of the 2012 July 12 CME from the Sun to the Earth: Data- Constrained Three-Dimensional MHD Simulations F. Shen 1, C. Shen 2, J. Zhang 3, P. Hess.
Solar Mass Ejection Imager (SMEI) Analysis of the 20 January 2005 CME B.V. Jackson, P.P. Hick, A. Buffington, M.M. Bisi, and E.A. Jensen Center for Astrophysics.

Solar Mass Ejection Imager (SMEI) Analysis of the 20 January 2005 CME B.V. Jackson, P.P. Hick, A. Buffington, M.M. Bisi, and E.A. Jensen Center for Astrophysics.
Solar System Physics Group Heliospheric physics with LOFAR Andy Breen, Richard Fallows Solar System Physics Group Aberystwyth University Mario Bisi Center.

Solar System Physics Group Heliospheric physics with LOFAR Andy Breen, Richard Fallows Solar System Physics Group Aberystwyth University Mario Bisi Center.
Space Weather from Coronal Holes and High Speed Streams M. Leila Mays (NASA/GSFC and CUA) SW REDISW REDI 2014 June 2-13.

Space Weather from Coronal Holes and High Speed Streams M. Leila Mays (NASA/GSFC and CUA) SW REDISW REDI 2014 June 2-13.
Comparison of the 3D MHD Solar Wind Model Results with ACE Data 2007 SHINE Student Day Whistler, B. C., Canada C. O. Lee*, J. G. Luhmann, D. Odstrcil,

Comparison of the 3D MHD Solar Wind Model Results with ACE Data 2007 SHINE Student Day Whistler, B. C., Canada C. O. Lee*, J. G. Luhmann, D. Odstrcil,
Upgrade of STEL Multi-Station Interplanetary Scintillation System and Recent Observations of the Solar Wind Munetoshi Tokumaru, Masayoshi Kojima, Ken ’

Upgrade of STEL Multi-Station Interplanetary Scintillation System and Recent Observations of the Solar Wind Munetoshi Tokumaru, Masayoshi Kojima, Ken ’

Similar presentations

Ads by Google