What’s happened to our Solar Minimum? H. Hudson

Slides:



Advertisements
Similar presentations
A Comparative Study of Searching Korean Scripts in OPACs: The Impact of Spaces Miree Ku Duke University.
Advertisements

Discussion of Paper THE MAUNDER MINIMUM IS NOT AS GRAND AS IT SEEMED TO BE N. V. Zolotova and D. I. Ponyavin Leif Svalgaard Stanford University Feb. 17,
Comparison of the Sun, Earth and Moon Earth Moon Sun Earth Moon.
The Solar Radio Microwave Flux and the Sunspot Number Leif Svalgaard Stanford University, Stanford, CA, USA. [ Hugh S Hudson University.
Bach ground: The correlation between sunspot proper motion and flares has been investigated for a long time (e.g. Antalova, 1965, Gesztelyi, 1984). The.
Microwave fluxes in the recent solar minimum H. Hudson, L. Svalgaard, K. Shibasaki, K. Tapping The time series of solar microwave flux traditionally is.
Sixty+ Years of Solar Microwave Flux Leif Svalgaard Stanford University SHINE 2010, Santa Fe, NM.
CAUSE OF ‘THE PAUSE’ IN GLOBAL WARMING: ITS IMPLICATIONS FOR FUTURE CLIMATES- THE PAST IS THE KEY TO THE FUTURE Don J. Easterbrook Dept. of Geology Western.
Hard X-rays associated with CMEs H.S. Hudson, UCB & SPRC Y10, Jan. 24, 2001.
Solar and Stellar Flares Hugh S. Hudson SSL, UC Berkeley 1 May
Solar Lunch Stuff H. Hudson. Malanushenko talk New approach to field extrapolation Use of image signatures in the volume to be mapped Iterative reconciliation.
ISSI THz Overview Hugh Hudson, Säm Krucker, Gerard Trottet.
Changyi Tan et al. NJIT, April 2008 Evolution of Evershed and Shear Flows Associated with the X3.4 Flare of 2006 December 13 Evolution of Evershed and.
More on Functions and Their Graphs Section 1.3. Objectives Calculate and simplify the difference quotient for a given function. Calculate a function value.
Energetic neutral atoms from solar flares H. S. Hudson SSL, UC Berkeley.
August 2006 IAU Assembly Halo CMEs and Configuration of Magnetic Field Yang Liu – Stanford University
Flare, SEP, and spot occurrence patterns: RHESSI astrobiology? H. Hudson Space Sciences Lab, UC Berkeley Featuring figures from a recently submitted -
The hard X-ray spectral structure of flare ribbons H. Hudson, L. Fletcher, S. Krucker, J. Pollock.
Solar Activities and Halloween Storms Ahmed Hady Astronomy Department Cairo University, Egypt.
Stanford, January Solar flares, magnetars, and helioseismology H.S. Hudson SSL/UCB.
RHESSI/NESSIE, June 2003 H.S. Hudson Gamma-ray event statistics H. Hudson, R. Lin, D. Smith.
Terahertz Flares H. S. Hudson SSL, UC Berkeley. SPD May 27, 2008 THz spectrum for solar studies Passbands at 0.2, 0.35, 0.67, 0.86 at best (driest) sites.
Coronal Hard X-rays Come of Age H. S. Hudson SSL, UC Berkeley.
B3 B1 B7 B2 B5 B4 B6 Which interfaces to keep and which to ignore. Pretend that the objective is to route to root (the one with smallest ID) and use least.
Long-Term Solar Variability H. S. Hudson University of California, Berkeley SORCE Science Meeting Sonoma, Dec. 6, 2003.
MDI Level 1.8 Magnetograms Yang Liu Stanford University 6/23/ SHINE 2008.
Prediction on Time-Scales of Years to Decades Discussion Group A.
1 Long-term Solar Synoptic Measurements with Implications for the Solar Cycle Leif Svalgaard Stanford University 23 April 2013.
1 Heliospheric Magnetic Field Leif Svalgaard Stanford University, CA
05, July, 2012, Moscow Session: SH ID: rd European Cosmic Ray Symposium Registration of Forbush decrease 2012/03/08 with a global net of the thermal.
Flares in and their associations with CMEs N.V. Nitta, J.P.Wuelser, M. J. Aschwanden, J. R. Lemen (LMSAL), D. M. Zarro (Adnet, Inc.)
The Unprecedented Solar Magnetic Fields and Their Implications December 21, 2009 Yu Yi Dept. of Astronomy & Space Science, Chungnam National University.
The day after solar cycle 23 IHY 2009 September 23, 2009 Yu Yi 1 and Su Yeon Oh 2 1 Dept. of Astronomy & Space Science, Chungnam National University, Korea.
Module Interpreting Real Gross Domestic Product KRUGMAN'S MACROECONOMICS for AP* 11 Margaret Ray and David Anderson.
1 The Spots That Won’t Form Leif Svalgaard Stanford University 3 rd SSN Workshop, Tucson, AZ, Jan
Spectral Properties of Heavy Ions Associated with Interplanetary Shocks at 1 AU SHINE 2004 Big Sky, Montana M. I. Desai University of Maryland, College.
Goal: To understand binary stars Objectives: 1)To review why we get binary star systems 2)To learn about the 2 different binary star types and how we find.
Limits and Derivatives 2. The Limit of a Function 2.2.
1 Large Solar Events in Historical Context Leif Svalgaard HEPL, Stanford University AGU Fall 2013, SH23D-02.
How efficient modern solar cells work. Jyunpei Y amamoto.
Identifying the Role of Solar-Wind Number Density in Ring Current Evolution Paul O’Brien and Robert McPherron UCLA/IGPP.
1 PMOD TSI: SOHO keyhole effect, and possible degradation over time Leif Svalgaard Stanford University, CA SORCE.
The Moon By the awesome J.J.. What would happen with no moon? Orpheus crashes into earth. Then a big explosion.
Solar Cycle Variation of the Heliospheric Magnetic Flux, Solar Wind Flux and Galactic Cosmic Rays Charles W. Smith, Nathan A. Schwadron Ken G. McCracken,
Reconstruction of the solar activity in 7th-11th centuries by the carbon 14 content in tree-rings F USA M IYAKE 1, K ENTARO N AGAYA 1, K IMIAKI M ASUDA.
Copyright © 2010 Terry Hudson Chapter 4 PLANNING & WRITING YOUR RESEARCH PAPER.
Smoke Example fires over Greece on 26 August 2007 Daniel Rosenfeld, MTG user consultation workshop, December 2007.
1 Rudolf Wolf Was Right Leif Svalgaard Stanford University Dec 9 th 2009 Seminar at UC Berkeley Space Sciences Lab.
The Ray Model of Light. Light and Matter Light is represented as straight lines called rays, which show the direction that light travels. Ray diagrams.
What do we Know of Solar Flares?
WSM Whole Sun Month Sarah Gibson If the Sun is so quiet, why is the Earth still ringing?
1 ~130 Years of Solar Wind Data: The Floor and More E.W. Cliver Space Vehicles Directorate Air Force Research Laboratory AGU May 2008.
Ahmed A. HADY Astronomy Department Cairo University Egypt Deep Solar Minimum of Cycle23 and its Impact and its Impact.
What the Long-Term Sunspot Record Tells Us About Space Climate David H. Hathaway NASA/MSFC National Space Science and Technology Center Huntsville, AL,
Diary of a Wimpy Cycle David H. Hathaway 1 and Lisa Upton 2,3 1 NASA/Marshall Space Flight Center/Science Research Office 2 Vanderbilt University 3 University.
Alexandre José de Oliveira e Silva(UNIVAP)
Introduction to Programming for Mechanical Engineers (ME 319)
Developing Sunspot March 27
Geomagnetic activity indicates large amplitude for sunspot cycle 24
Bell Ringer Sometimes during an eclipse of the moon (lunar eclipse), only part of the moon we see is blocked. Other times, the entire moon we see is blocked.
MDI Global Field & Solar Wind
The Sun Chapter 17.
3.2 – Concavity and Points of Inflection
~130 Years of Solar Wind Data: The Floor and More
Forbush and GCRDs First rigorous experimental observation of Cosmic Ray Flux Decrease was obtained by S. E. Forbush in , after deep statisitcal.
Chapter 16: Other Descriptive Research Methods
OVERALL STATUS OF THE TESTING EXERCISE
Resource by Katie Hudson
2.2 The Limit of a Function.
Solution to Problem 2.25 DS-203 Fall 2007.
Presentation transcript:

What’s happened to our Solar Minimum? H. Hudson

SSL March 11, /5

SSL March 11, /5 Leif Svalgaard’s view of “Now” Where do the minima in TSI come from? Is F10.7 now showing an increase; if so, what is the mechanism? Why doesn’t TSI correlate with the wee spots that do appear?

SSL March 11, /5 F10.7 comparisons of minima

SSL March 11, /5 Conclusions Viewed simplistically on just the basis of F10.7, we are many sigma overdue The behavior of the standard indices during the minimum does is not following the script very well For  -ray flare occurrence, it may not matter much - see ApJ 663, L45 (2007)