SOHO experiment Proton Differential Fluxes, 2-hour averages

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Interface to produce plots, listings or output files

Scatter plot for definitive 1-hr res. Fluxes from SOHO ERNE Experiment

Original 1-min data source at https://srl.utu.fi/export/
Only arithmetic averaging was done for calculating of hourly data . (No averaging of logarithms and No threshold numbers of finer scale points.) We believe, these data will be useful for looking at large solar disturbances near Earth.

Time span: 1996-05-07 - 2024-11-07

Please enter your selections and then click on the Submit button.

Scatter plot/regression fit (max # points = 30000) List data

Enter start and stop dates: year,month,day(YYYYMMDD) or year,day_of_year(YYYYDOY)
Start time Stop time

Select X and Y variables
Fluxes are given in 1/(sec-cm**2-ster-MeV/n );

Select X and Y variables bins arein MeV/n

Protons(H)

1.3- 1.6 X Y

1.6- 2.0 X Y

2.0- 2.5 X Y

2.5- 3.2 X Y

3.2- 4.0 X Y

4.0- 5.0 X Y

5.0- 6.4 X Y

6.4- 8.0 X Y

8.0- 10. X Y

10.- 13. X Y

13- 16 X Y

16- 20 X Y

20- 25 X Y

25- 32 X Y

32- 40 X Y

40- 50 X Y

50- 64 X Y

64- 80 X Y

80- 100 X Y

100- 130 X Y

Helium(He4)

1.3- 1.6 X Y

1.6- 2.0 X Y

2.0- 2.5 X Y

2.5- 3.2 X Y

3.2- 4.0 X Y

4.0- 5.0 X Y

5.0- 6.4 X Y

6.4- 8.0 X Y

8.0- 10. X Y

10.- 13. X Y

13- 16 X Y

16- 20 X Y

20- 25 X Y

25- 32 X Y

32- 40 X Y

40- 50 X Y

50- 64 X Y

64- 80 X Y

80- 100 X Y

100- 130 X Y

Select the fitting method
No fitting Delta-Y method(N<30000)

Advanced plot selections (optional)

X-axes type:	Y-axes type:
	Character size (0.5-2.0):
Plot symbol:	Symbol size (0.1-4.0):
Image size (pixels): X: Y:	Connect style:

If you have any questions/comments about the OMNWeb Plus, contact Dr. Natalia Papitashvili,Mail Code 672, NASA/Goddard Space Flight Center, Greenbelt, MD 20771

NASA Official: Robert Candey (Robert.M.Candey@nasa.gov), Head of the Space Physics Data Facility