File:Graph of sunspot numbers between 1610-1990. More sunspots generally mean more energy received by the Earth (NASA).png
Graph_of_sunspot_numbers_between_1610-1990._More_sunspots_generally_mean_more_energy_received_by_the_Earth_(NASA).png (576 × 104 pixels, file size: 11 KB, MIME type: image/png)
File information
Structured data
Captions
Summary edit
DescriptionGraph of sunspot numbers between 1610-1990. More sunspots generally mean more energy received by the Earth (NASA).png |
English: Graph of sunspot numbers between 1610-1990. The graph is by Robert Simmon, based on data from Hoyt and Schatten (1997) (referred to by Riebeek, 2010). Data from Hoyt and Schatten (1997) can be downloaded from the NGDC (2009). From the cited Riebeek (2010) public-domain source: "Records of sunspots dating back to 1610 provide an indication of energy output from the Sun. In general, more sunspots (blue peaks) mean more intense solar activity and more energy received by the Earth. On average, there are more sunspots now than during the Maunder Minimum 350 years ago, but the increase in solar activity alone is not sufficient to explain the temperature increases that have occurred since 1950." For more information, see attribution of recent climate change. References:
|
Date | |
Source | sunspots_narrow.png, in: Has the Sun been more active in recent decades, and could it be responsible for some global warming? (Riebeek, H., June 24, 2010), part of: Climate Q&A : Blogs. Publisher: Earth Observatory, part of the EOS Project Science Office, located at NASA Goddard Space Flight Center. |
Author | Robert Simmon |
Permission (Reusing this file) |
Image Use Policy: "Most materials published on the Earth Observatory, including images, are freely available for re-publication or re-use, including commercial purposes, with the following exceptions: *where copyright is indicated, you must obtain the copyright holder’s permission; we usually provide links to the organization that holds the copyright, *images from the SeaWiFS sensor older than five years are in the public domain and can be re-used or re-published for any purpose. Images less than five years old can be re-used only for educational or scientific purposes; any commercial use of such images must be coordinated with GeoEye. We ask that NASA’s Earth Observatory be given credit for its original materials; the only mandatory credit is NASA." |
Licensing edit
Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
Warnings:
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 05:36, 27 October 2012 | 576 × 104 (11 KB) | Enescot (talk | contribs) | {{Information |Description ={{en|1=Graph of sunspot numbers between 1610-1990. The graph is by Robert Simmon, based on data from Hoyt and Schatten (1997) (referred to by Riebeek, 2010). Data from Hoyt and Schatten (1997) can be downl... |
You cannot overwrite this file.
File usage on Commons
There are no pages that use this file.
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Horizontal resolution | 28.35 dpc |
---|---|
Vertical resolution | 28.35 dpc |