Why a Sun-Earth line Coronagraph is Best Doug Biesecker NOAA/SWPC.

Slides:



Advertisements
Similar presentations
Heliospheric Propagation of ICMEs: The Drag-Based Model B. Vršnak 1, T. Žic 1, M. Dumbović 1, J. Čalogović 1, A. Veronig 2, M. Temmer 2, C. Moestl 2, T.
Advertisements

Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.
CAS Key Laboratory of Geospace Environment, USTC The Deflection of 2008 September 13 CME in Heliosphere Space ISEST, Hvar, Croatia,2013 June 17 Collaborators:
Interaction of coronal mass ejections with large-scale structures N. Gopalswamy, S. Yashiro, H. Xie, S. Akiyama, and P. Mäkelä IHY – ISWI Regional meeting.
Reviewing the Summer School Solar Labs Nicholas Gross.
SWPC CME Imaging Requirements for the post-SOHO era Douglas Biesecker 3/25/2014.
Assessing the Contribution of Heliospheric Imaging in Improving Space Weather Prediction SHINE Session 6 Simon Plunkett and Doug Biesecker Thursday Morning.
Resolving the 180 Degree Ambiguity in Vector Magnetic Fields T. Metcalf.
E. Robbrecht – SIDC- Royal Observatory of Belgium 8 March 2007 The statistical importance of narrow CMEs Open questions to be addressed by SECCHI Eva Robbrecht,
Specification of the broad shell of dense plasma for halo CMEs Xuepu Zhao Stanford University Stanford University EGU Session ST2 Vienna, Austria 25 April.
The Hunt for a Link : Quantitative Connections Between Magnetic Fields and EIT Coronal Wave/CME Properties Prepared by James R. Robertson J.R. In conjunction.
1 Determination of 3D CME Trajectories using Stereoscopy Paulett Liewer, Jeff Hall, Eric DeJong, JPL Vahab Pournaghsband, UCB Arnaud Thernisien and Russ.
CME-driven Shocks in White Light Observations SOHO/LASCO C3 – CME May 5 th, 1999 CME-driven Shock We demonstrate that CME-driven shocks: (1) can be detected.
My 20 Years of Service at Stanford Solar Physics Group I. Improvement of inner boundary condition for data-based coronal models (WSO, MDI, HMI). II. Development.
3D Stereoscopic Reconstruction of CMEs by Forward Modeling 5th Consortium STEREO-SECCHI Meeting Orsay, March 2007 Y.BOURSIER – P.LAMY – F.GOUDAIL - A.LLEBARIA.
C. May 12, 1997 Interplanetary Event. Ambient Solar Wind Models SAIC 3-D MHD steady state coronal model based on photospheric field maps CU/CIRES-NOAA/SEC.
ZEC Model parameters of Halo CMEs Xuepu Zhao Jan. 18, 2011.
Improvement of Inversion Solutions for Type C Halo CMEs Using the Elliptic Cone Model.
R F For a central force the position and the force are anti- parallel, so r  F=0. So, angular momentum, L, is constant N is torque Newton II, angular.
The global character of the Earth-directed coronal mass ejection and its trigger Xuepu Zhao and J. Todd Hoeksema Stanford University The Firs.
C. May 12, 1997 Interplanetary Event. May 12, 1997 Interplanetary Coronal Mass Ejection Event CU/CIRES, NOAA/SEC, SAIC, Stanford Tatranska Lomnica, Slovakia,
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.
The First Space-Weather Numerical Forecasting Model & Reconstruction of Halo CMEs Xuepu Zhao NAOC Oct.
Determination of Geometrical and Kinematical Properties of Disk Halo CMEs Using the Elliptic Cone Model X. P. Zhao, H. Cremades, J. T. Hoeksema, Y. Liu.
Longitude and Latitude
RT Modelling of CMEs Using WSA- ENLIL Cone Model
Characterization of Coronal Mass Ejection Deflection using Coronagraph Image Sequences Jenna L. Zink, GMU Undergraduate Research Scholars Program, Rebekah.
1 Interpreting SECCHI White Light Images: FOV Sensitivity & Stereo Viewing Paulett Liewer, JPL; Russ Howard & Dennis Socker, NRL SECCHI Consortium Meeting.
Assessing Predictions of CME Time- of-Arrival and 1 AU Speed to Observations Angelos Vourlidas Vourlidas- SHINE
A Catalog of Halo Coronal Mass Ejections from SOHO N. Gopalswamy 1, S. Yashiro 2, G. Michalek 3, H. Xie 3, G. Stenborg 2, A. Vourlidas 4, R. A. Howard.
1 Determination of CME 3D Trajectories using COR Stereoscopy + Analysis of HI1 CME Tracks P. C. Liewer, E. M. DeJong, J. R. Hall, JPL/Caltech; N. Sheeley,
Solar Drivers of Space Weather Steven Hill NOAA/SEC June 14, 2007 Research Experience for Undergraduates.
Θ θ 45 - θ θ b a r s Mirror diameter = D Focal ratio = F Focal length = a + b Major axis = r + s tan θ = D / 2(a+b) = 1 / 2F D b tan θ.
Kinematics in 2-D Concept Map
Properties of Stars.
K9LA Vancouver 2003 Disturbances to Propagation Carl Luetzelschwab K9LA CQ DX?Where’d everybody go?
Arrival time of halo coronal mass ejections In the vicinity of the Earth G. Michalek, N. Gopalswamy, A. Lara, and P.K. Manoharan A&A 423, (2004)
Stars: Binary Systems. Binary star systems allow the determination of stellar masses. The orbital velocity of stars in a binary system reflect the stellar.
Questions that we are facing in forecasting CME’s arrival Yuming Wang & Chenglong Shen STEP USTC Croatia.
EumetCal Examples.
Lessons for STEREO - learned from Helios Presented at the STEREO/Solar B Workshop, Rainer Schwenn, MPS Lindau The Helios.
Forecast of Geomagnetic Storm based on CME and IP condition R.-S. Kim 1, K.-S. Cho 2, Y.-J. Moon 3, Yu Yi 1, K.-H. Kim 3 1 Chungnam National University.
-1- Coronal Faraday Rotation of Occulted Radio Signals M. K. Bird Argelander-Institut für Astronomie, Universität Bonn International Colloquium on Scattering.
The Organization of the Solar System and Planetary Motion
11. Assessing the Contribution of Heliospheric Imaging, IPS and other remote sensing observations in Improving Space Weather Prediction Bernie Jackson,
Improving Space Weather Forecasts Using Coronagraph Data S.P. Plunkett 1, A. Vourlidas 1, D.R. McMullin 2, K. Battams 3, R.C. Colaninno 4 1 Naval Research.
6.1 Gravitational fields State Newton’s universal law of gravitation Define gravitational field strength Determine the gravitational.
Angular Separation is not enough! We want to know the answer to the ‘age old question’: How far away are the stars? Ans: A lot farther than anyone imagined!
Part 2: CME Analysis with StereoCAT for Space Weather: Limitations Barbara Thompson (NASA/GSFC) (presented by Leila Mays)
Solar Wind Propagation Tool Chihiro Tao 1,2, Nicolas Andre 1, Vincent Génot 1, Alexis P. Rouillard 1, Elena Budnik 1, Arnaud Biegun 1, Andrei Fedorov 1.
Analysis of 3 and 8 April 2010 Coronal Mass Ejections and their Influence on the Earth Magnetic Field Marilena Mierla and SECCHI teams at ROB, USO and.
A tool for improved space weather predictions: the CME expansion speed. Max-Planck-Institut für Aeronomie Katlenburg-Lindau Germany Instituto Nacional.
Shocks in the IPS Wageesh Mishra Eun-kyung Joo Shih-pin Chen.
Celestial Mechanics I Introduction Kepler’s Laws.
Multi-Point Observations of The Solar Corona for Space weather Acknowledgements The forecasting data was retrieved from NOAA SWPC products and SIDC PRESTO.
The CME geomagnetic forecast tool (CGFT) M. Dumbović 1, A. Devos 2, L. Rodriguez 2, B. Vršnak 1, E. Kraaikamp 2, B. Bourgoignie 2, J. Čalogović 1 1 Hvar.
1 Pruning of Ensemble CME modeling using Interplanetary Scintillation and Heliospheric Imager Observations A. Taktakishvili, M. L. Mays, L. Rastaetter,
October-November CMEs Yang Liu – Stanford University
Detecting, forecasting and modeling of the 2002/04/17 halo CME Heliophysics Summer School 1.
How do we locate objects in the sky? Angular separation: the angle between objects as seen from Earth (Degrees are separated into minutes (60 minutes of.
Towards unambiguous characterization of coronal structures
Met Office Forecaster and Customer Requirements and Rationale
Solar & Lunar Eclipses.
Orientations of Halo CMEs and Magnetic Clouds
Solar & Lunar Eclipses.
Corona Mass Ejection (CME) Solar Energetic Particle Events
Forecasting the arrival time of the CME’s shock at the Earth
Chapter 4A: SOLAR RADIATION- GEOMETRY
SOHO images of eruptive flares (left) on Nov. 6, 2004
Chapter 4A: SOLAR RADIATION- GEOMETRY
Presentation transcript:

Why a Sun-Earth line Coronagraph is Best Doug Biesecker NOAA/SWPC

Outline Use classic Full Halo, Partial Halo, Limb morphology to determine Earth impact – Need secondary observations to resolve near side - far side ambiguity X-ray flare, X-ray/EUV image, H-alpha image Classic cone model can be used to derive CME parameters needed to drive WSA-Enlil – Need a constraint on CME width – Right now, more than one view is required, but there is hope CME’s seen from the side have longitude ambiguity at least, and are unresolved at worst – Don’t know if Earth will get hit by the CME – Will polarization data resolve this? Is there a preferred angular separation?

Limb CME Headed away from Earth Definite miss No geomagnetic storm Partial Halo CME Glancing blow at Earth Probable hit – Harder to predict Weaker, shorter geomagnetic storm Headed directly at the Earth Definite hit Strongest, longest geomagnetic storm Halo CME Classic CME Descriptions

longitude radial velocity latitude radius CME ‘Cone’ Geometry CME parameters calculated from analysis of SOHO images Xie et al b a h α

Latitude (deg)Longitude (deg)Cone ½ Angle (deg) Radial distance (Rs) b c d e f Problem: Which ellipse ?

Problem: Ellipses are “freeform” – no constraints on eccentricity vs offset Cone ½ Angle = 83 degrees (full Angle 166 !!)

Full 3D graphics solution – can only represent ‘correct’ cones originating at the Sun Need to know the cone angle Big problem since cone angle inversely proportional to velocity (roughly)

Cone ½ Angle 30 degrees45 degrees60 degrees factor 2 difference in velocity Again: Which ellipse ?

What if we only have one Coronagraph ?

If only one side view… Answers below vary depending on s/c-Sun- Earth angle – CME latitude is well determined – CME Width and Earthward velocity are usually well determined, though can still be problematic – CME longitude remains ambiguous, if not unknown – Radial propagation is a bad assumption Need to test this – I have the data to do so

POS Ambiguity is the difference between a hit and a miss Is it possible to tell the difference Between a Full and partial Halo? A single side view always has problems

CME Analysis Tool (CAT)