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BRITISH GEOLOGICAL SURVEY Port Stanley Observatory Monthly Magnetic Bulletin July 2010 10/07/PS Jason Islands a ar C West Falkland Kin gg eor ge B Port Salavador ay Weddell Island Mount Osborne So un d 700m eb an d rlot t Mount Adam Sapper Hill Berkley Sound 705m Goose Green lkl Cha ay Fa Qu een nd d nd an Isl Isla l rs e e p d un Kep Sa sla si s ca Stanley Darwin Choiseul Sound Port Stephens Bay of Harbours Eag le P East Falkland ass age Crown copyright; Ordnance Survey

PORT STANLEY OBSERVATORY MAGNETIC DATA 1. Introduction Port Stanley observatory was installed by the British Geological Survey (BGS) with financial support from a consortium of oil companies and became operational in February 1994. This bulletin is published to provide rapid access to the provisional geomagnetic observatory results. The information is freely available for personal, academic, educational and non-commercial research or use. Magnetic observatory data are presented as a series of plots of one-minute, hourly and daily values, followed by tabulations of monthly values. The operation of the observatory and presentation of data are described in the rest of this section. Enquiries about the data should be addressed to: 2. Position Geomagnetism Team Earth Hazards and Systems British Geological Survey Murchison House, West Mains Road Edinburgh EH9 3LA Scotland, UK Tel: +44 (0) 131 667 1000 Fax: +44 (0) 131 650 0265 E-mail: enquiries@bgs.ac.uk Internet: www.geomag.bgs.ac.uk Port Stanley Observatory, one of the geomagnetic observatories maintained and operated by the British Geological Survey (BGS), is situated on a site at Sapper Hill near Port Stanley in the Falkland Islands. The observatory co-ordinates are: Geographic: 51.704 S 302.107 E Geomagnetic: 42.005 S 11.942 E Height above mean sea level: 135 m The geomagnetic co-ordinates are approximations, calculated using the 11th generation International Geomagnetic Reference Field (IGRF) at epoch 2010.5. On-line access to models (including IGRF), charts and navigational data are available at www.geomag.bgs.ac.uk/navigation.html 3. The Observatory Operation 3.1 GDAS The observatory operates under the control of the Geomagnetic Data Acquisition System (GDAS), which was developed by BGS staff, installed and became operational in August 2002. The data acquisition software, running on QNX operated computers, controls the data logging and the communications. There are two sets of sensors used for making magnetic measurements. A tri-axial linear-core fluxgate magnetometer, manufactured by the Danish Meteorological Institute, is used to measure the variations in the horizontal (H) and vertical (Z) components of the field. The third sensor is oriented perpendicular to these, and measures variations, which are proportional to the changes in declination (D). Measurements are made at a rate of 1 Hz. In addition to the fluxgate sensors there is a proton precession magnetometer (PPM) making measurements of the absolute total field intensity (F) at a rate of 0.1Hz. The raw unfiltered data are retrieved automatically via Internet connections to the BGS office in Edinburgh in near real-time. The fluxgate data are filtered to produce one-minute values using a 61- point cosine filter and the total field intensity samples are filtered using a 7-point cosine filter. The one-minute values provide input for various data products in the Geomagnetism Information and Forecast Service (GIFS), available on-line at www.geomag.bgs.ac.uk/on_line_gifs.html 3.2 Absolute Observations The GDAS fluxgate magnetometers accurately measure variations in the components of the geomagnetic field, but not the absolute magnitudes. Two sets of absolute measurements of the field are made manually twice per month. A fluxgate sensor mounted on a theodolite is used to determine D and inclination (I); the GDAS PPM measurements, with a site difference correction applied, are used for F. The absolute observations are used in conjunction with the GDAS variometer measurements to produce a continuous record of the absolute values of the geomagnetic field elements as if they had been measured at the observatory reference pillar.

4. Observatory Results The data presented in the bulletin are in the form of plots and tabulations described in the following sections. 4.1 Absolute Observations The absolute observation measurements made during the month are tabulated. Also included are the corresponding baseline values, which are the differences between the absolute measurements and the variometer measurements of D, H and Z (in the sense absolute variometer). These are also plotted (markers) along with the derived preliminary daily baseline values (line) throughout the year. Daily mean differences between the measured absolute F and the F computed from the baseline corrected H and Z values are plotted in the fourth panel (in the sense measured derived). The bottom panel shows the daily mean temperature in the fluxgate chamber. 4.2 Summary magnetograms Small-scale magnetograms are plotted which allow the month's data to be viewed at a glance. They are plotted 16 days to a page and show the one-minute variations in D, H and Z. The scales are shown on the right-hand side of the page. On disturbed days the scales are multiplied by a factor, which is indicated above the panel for that day. The variations are centred on the monthly mean value, shown on the left side of the page. 4.3 Magnetograms The daily magnetograms are plotted using oneminute values of D, H and Z from the fluxgate sensors, with any gaps filled using back-up data. The magnetograms are plotted to a variable scale; scale bars are shown to the right of each plot. The absolute level (the monthly mean value) is indicated on the left side of the plots. quiet intervals. Plotting the data in this way highlights this recurrence. Diurnal variations are also clear in these plots and the amplitude changes throughout the year highlight the seasonal changes. Longer term secular variation is also illustrated. 4.5 Daily and Monthly Mean Values Daily mean values of D, H, Z and F are plotted throughout the year. In addition, a table of monthly mean values of all the geomagnetic elements is provided. These values depend on accurate specification of the fluxgate sensor baselines. It is anticipated that these provisional values will not be altered by more than a few nt or tenths of arcminutes before being made definitive at the end of the year. 5. Conditions of Use The data presented in this bulletin are provided for personal, academic, educational, non-commercial research or other non-commercial use and are not for sale or distribution to third parties without written permission from BGS. Reproduction of any part of this bulletin should be accompanied by the statement: 'Reproduced with the permission of the British Geological Survey NERC. All rights Reserved'. Publications making use of the data should include an acknowledgment statement of the form: The results presented in this paper rely on the data collected at Port Stanley magnetic observatory, operated by the British Geological Survey. Commercial users can contact the geomagnetism team for information on the range of applications and services offered. Full contact details are available at www.geomag.bgs.ac.uk/staff.html. 4.4 Hourly Mean Value Plots Hourly mean values of D, H and Z for the past 12 months are plotted in 27-day segments corresponding to the Bartels solar rotation number. Magnetic disturbances associated with active regions and/or coronal holes on the Sun may recur after 27 days: the same is true for geomagnetically NERC 2010. All rights reserved Edinburgh British Geological Survey 2010

PORT STANLEY OBSERVATORY ABSOLUTE OBSERVATIONS Date Day Number Time (UT) Declination Inclination Total Field Horizontal Intensity Vertical Intensity Absolute (º) Baseline (º) Time (UT) Absolute (º) Site difference (nt) Absolute corrected (nt) 04-Jul-10 185 18:03 3.4165 3.6583 18:13-49.4065-32.6 28722.6 18689.4 18848.0-21810.4-21940.5 NB 04-Jul-10 185 18:22 3.4098 3.6583 18:33-49.4058-32.6 28722.4 18689.6 18847.5-21810.0-21940.9 NB 17-Jul-10 198 19:01 3.1167 3.3650 19:10-49.4064-32.6 28726.6 18692.1 18847.2-21813.4-21941.4 NB 17-Jul-10 198 19:17 3.3955 3.6500 19:25-49.4042-32.6 28727.0 18693.2 18846.7-21813.0-21941.7 NB Absolute (nt) Baseline (nt) Absolute (nt) Baseline (nt) Observer

Falkland Island 2010 Declination : Absolute - Variometer (markers) and Baseline Applied (line) 219.1 5min Horizontal Intensity : Absolute - Variometer (markers) and Baseline Applied (line) 18848 Vertical Intensity : Absolute - Variometer (markers) and Baseline Applied (line) -21940 Total Intensity : Absolute (Proton F) - Baseline Adjusted Variometer (derived F) 32.6 Temperature Inside Variometer Hut 23.2 20 C Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec

July 2010 1 2 3 4 D 0.50 o H Z 5 6 7 8 D H 150 nt Z 9 10 11 12 D H Z 150 nt 13 14 15 16 D H Z 6 12 18 24 6 12 18 24 6 12 18 24 6 12 18 24

17 18 19 20 D 0.50 o H Z 21 22 23 24 D H 150 nt Z 25 26 27 28 D H Z 150 nt D 29 30 31 6 12 18 24 UT H Z 6 12 18 24 6 12 18 24 6 12 18 24 July 2010

Date: 01-07-2010 Day number: 182 Date: 02-07-2010 Day number: 183

Date: 03-07-2010 Day number: 184 Date: 04-07-2010 Day number: 185

Date: 05-07-2010 Day number: 186 Date: 06-07-2010 Day number: 187

Date: 07-07-2010 Day number: 188 Date: 08-07-2010 Day number: 189

Date: 09-07-2010 Day number: 190 Date: 10-07-2010 Day number: 191

Date: 11-07-2010 Day number: 192 Date: 12-07-2010 Day number: 193

Date: 13-07-2010 Day number: 194 Date: 14-07-2010 Day number: 195

Date: 15-07-2010 Day number: 196 40nT 30nT Date: 16-07-2010 Day number: 197

Date: 17-07-2010 Day number: 198 Date: 18-07-2010 Day number: 199

Date: 19-07-2010 Day number: 200 Date: 20-07-2010 Day number: 201

Date: 21-07-2010 Day number: 202 Date: 22-07-2010 Day number: 203

Date: 23-07-2010 Day number: 204 Date: 24-07-2010 Day number: 205

Date: 25-07-2010 Day number: 206 Date: 26-07-2010 Day number: 207

Date: 27-07-2010 Day number: 208 30nT Date: 28-07-2010 Day number: 209 30nT

Date: 29-07-2010 Day number: 210 Date: 30-07-2010 Day number: 211

Date: 31-07-2010 Day number: 212

Observatory: Declination (degrees) 3.52 Rotn 3.31 2401 Aug09 2402 Sep 2403 Oct 2404 Nov 2405 Dec 2406 Jan10 2407 Feb 2408 Mar 2409 Apr 2410 May 2411 2412 Jun 2413 Jul 2414 2415 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 Hourly Mean Values Plotted By Bartels Solar Rotation Number

Observatory: Horizontal Intensity (nt) 18796 Rotn 18655 2401 Aug09 2402 Sep 2403 Oct 2404 Nov 2405 Dec 2406 Jan10 2407 Feb 2408 Mar 2409 Apr 2410 May 2411 2412 Jun 2413 Jul 2414 2415 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 Hourly Mean Values Plotted By Bartels Solar Rotation Number

Observatory: Vertical Intensity (nt) -21799 Rotn -21843 2401 Aug09 2402 Sep 2403 Oct 2404 Nov 2405 Dec 2406 Jan10 2407 Feb 2408 Mar 2409 Apr 2410 May 2411 2412 Jun 2413 Jul 2414 2415 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 Hourly Mean Values Plotted By Bartels Solar Rotation Number

Falklands Is Observatory 2010 Daily Mean Declination (deg) 204.0 10min Daily Mean Horizontal Intensity (nt) 18706 100nT Daily Mean Vertical Intensity (nt) -21816 50nT Daily Mean Total Intensity (nt) 28738 50nT Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec

Monthly Mean Values for Port Stanley Observatory 2010 Month D H I X Y Z F January 3 25.2 18738 nt -49 20.7 18704 nt 1118 nt -21820 nt 28761 nt February 3 24.9 18721 nt -49 22.3 18687 nt 1115 nt -21819 nt 28750 nt March 3 24.2 18715 nt -49 22.5 18682 nt 1111 nt -21815 nt 28743 nt April 3 24.1 18697 nt -49 24.4 18664 nt 1110 nt -21819 nt 28734 nt May 3 23.7 18695 nt -49 24.4 18662 nt 1107 nt -21817 nt 28731 nt June 3 23.2 18692 nt -49 24.4 18660 nt 1104 nt -21813 nt 28727 nt July 3 22.9 nt -49 24.3 18657 nt 1102 nt nt 28722 nt Note i. The values shown here are provisional.