1 Rudolf Wolf Was Right Leif Svalgaard Stanford University Dec 9 th 2009 Seminar at UC Berkeley Space Sciences Lab.

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Presentation transcript:

1 Rudolf Wolf Was Right Leif Svalgaard Stanford University Dec 9 th 2009 Seminar at UC Berkeley Space Sciences Lab.

2 The Sunspot Number(s) Wolf Number = k W (10*G + S) G = number of groups S = number of spots Group Number = 12 k G G Rudolf Wolf ( )Ken Schatten The ’12’ is to make the mean for the past ~100 years the same as the mean Wolf Number

3 The Number of Sunspot Groups is However also Observer Dependent SchwabeWolfCarringtonShea PetersSpoererWeberSchmidt SecchiBernaertsWolferAguilar RiccoRGO GSN = 12 k G Groups

4 The Problem: Discordant Sunspot Numbers Hoyt & Schatten, GRL 21, 1994

5 Wolf’s early SSNs were also low as the Group Numbers, but Wolf found a way of calibrating independently the SSN Was this justified?

6 Wolf’s Discovery: rD = a + b R W. H North X D Y = H sin(D) dY = H cos(D) dD For small dD rY Morning Evening East Y rD A current system in the ionosphere is created and maintained by solar FUV radiation

7 10 Days of geomagnetic variations rY

8 Definition of the Range, rY, of the Day-time variation of the Y-component. X points towards North, Y points towards East, Z points Downwards. The diurnal variation consists of two ‘waves’: 1) a day wave [the Sq current system] and 2) a weaker night wave of return currents from the auroral electrojets. There is a clear seasonal variation in the relative strength of the two current systems. We are only interested in the day wave

9 The clear solar cycle variation of rY All mid-latitude stations show the same variation, responding to the same current system This was Wolf’s justification for his calibration of the SSN

10 Solar Activity: Radio Flux at 2.8 GHz or 10.7 cm Very stable and well-determined from Canadian and Japanese stations

11 Using rY from nine ‘chains’ of stations we find that the correlation between F10.7 and rY is extremely good (more than 98% of the variation is accounted for) This establishes that Wolf’s procedure and calibration are physically sound

12 The diurnal range rY is thus an extremely good proxy for the F10.7 radio flux and [presumably] for ‘solar activity’ in general Here is the response at Helsinki and at its replacement station Nurmijarvi

13 We conclude that Wolf was justified in using the geomagnetic data to calibrate his sunspot number series and that the Group Sunspot Number does not represent a true picture of solar activity

14 No Long-Term Trend in TSI The justification for a long-term trend in Total Solar Irradiance is now largely gone. This may have implications for Climate Change due to the Sun.

15 Abstract The 'inventor' of the Sunspot Number [SSN], Rudolf Wolf, also discovered that the radiation from the Sun was controlling the daily variation of the compass needle [discovered by George Graham in 1722]. Wolf used this solar-terrestrial relationship to calibrate the Sunspot Number observed by many observers before Wolf's own observations and to bring all observers on to a common scale. After Wolf's death, later researchers forgot this and the sunspot number calibration drifted as even the counting method changed over time. Hoyt and Schatten's [H&S] Group Sunspot Number [GSN] also suffers from unknown calibration and H&S even concluded that Wolf's calibration was erroneous. The difference between the Wolf number, SSN, and the GSN at times amounts to a factor of two and has given rise to the Myth that we have just passed t 'Modern Grand Maximum' and that solar activity in recent cycles was the highest in ~10,000 years. We show that solar activity in the 20th century was not significantly different from the preceding two centuries and that Wolf was correct in his reconstruction of the SSN. That the GSN thus is not a correct representation of solar activity has severe impact on reconstructions and calibrations of several solar activity indicators, such as Total Solar Irradiance and Cosmic Rays proxies, with potential impact on modeling of Climate Change

16 Cosmic Ray Proxy 14 C and SSN For Q/A sesssion