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BRITISH GEOLOGICAL SURVEY Port Stanley Observatory Monthly Magnetic Bulletin May 2009 09/05/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 BGS with financial support from a consortium of oil companies and became operational in February 1994. This bulletin is published to meet the needs of users of geomagnetic data. Magnetic observatory data is presented as a series of plots of one-minute, hourly and daily values, followed by a tabulation 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 National Geomagnetic Service 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: orba@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. The observatory co-ordinates are: Geographic: 51 42.24 S 302 06.42 E Geomagnetic: 41 40.92 S 11 25.98 E Height above mean sea level: 135 m The geomagnetic co-ordinates are calculated using the 10th generation International Geomagnetic Reference Field at epoch 2009.5. 3. The Observatory Operation 3.1 GDAS The observatory operates under the control of the Geomagnetic Data Acquisition System (GDAS), developed by BGS, which was installed in August 2002. The system operates under the control of data acquisition software running on QNX computers, which control the data logging and communications. There are two sets of sensors used for making magnetic measurements. A triaxial 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 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 whilst the total field intensity samples are filtered using a 7-point cosine filter. 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 once per week. 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. Data Presentation 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 a page and show the 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 one-minute 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. 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 on the surface of the Sun may recur after 27 days: the same is true for geomagnetically quiet intervals. Plotting the data in this way highlights this recurrence, and also illustrates seasonal and diurnal variations throughout the year. 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. This data is provisional. It is anticipated that provisional values will not be altered by more than a few nt or tenths of arcminutes before being made definitive.

NERC 2009

PORT STANLEY OBSERVATORY ABSOLUTE OBSERVATIONS Date Day Number Time (UT) DECLINATION Absolute (º) Baseline (º) Time (UT) Inclination (º) Total Field Intensity (nt) INCLINATION H Absolute (nt) H Baseline (nt) Z Absolute (nt) Z Baseline (nt) 10-May-09 130 19:41 3.4934 3.6767 19:48-49.2677 28806.0 18796.7 18864.3-21828.2-21926.4 NB 10-May-09 130 19:56 3.4523 3.6400 20:05-49.2804 28805.4 18791.5 18859.3-21831.9-21930.7 NB 23-May-09 143 18:32 70 3.6450 18:39-49.3081 28802.5.0 18848.4-21838.8-21940.1 NB 23-May-09 143 18:47 3.4832 3.6517 18:54-49.3081 28803.6.7 18848.0-21839.6-21940.4 NB Observer

Falkland Island 2009 Declination : Absolute - Variometer (markers) and Baseline Applied (line) 219.2 5min Horizontal Intensity : Absolute - Variometer (markers) and Baseline Applied (line) 18848 Vertical Intensity : Absolute - Variometer (markers) and Baseline Applied (line) -21941 Total Intensity : Absolute (Proton F) - Baseline Adjusted Variometer (derived F) 31.0 Temperature Inside Variometer Hut 23.2 20 C Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec

May 2009 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 May 2009

Date: 01-05-2009 Day number: 121 Date: 02-05-2009 Day number: 122

Date: 03-05-2009 Day number: 123 Date: 04-05-2009 Day number: 124

Date: 05-05-2009 Day number: 125 Date: 06-05-2009 Day number: 126

Date: 07-05-2009 Day number: 127 Date: 08-05-2009 Day number: 128

Date: 09-05-2009 Day number: 129 30nT Date: 10-05-2009 Day number: 130

Date: 11-05-2009 Day number: 131 Date: 12-05-2009 Day number: 132

Date: 13-05-2009 Day number: 133 Date: 14-05-2009 Day number: 134

Date: 15-05-2009 Day number: 135 Date: 16-05-2009 Day number: 136

Date: 17-05-2009 Day number: 137 Date: 18-05-2009 Day number: 138

Date: 19-05-2009 Day number: 139 Date: 20-05-2009 Day number: 140

Date: 21-05-2009 Day number: 141 Date: 22-05-2009 Day number: 142

Date: 23-05-2009 Day number: 143 Date: 24-05-2009 Day number: 144

Date: 25-05-2009 Day number: 145 Date: 26-05-2009 Day number: 146

Date: 27-05-2009 Day number: 147 Date: 28-05-2009 Day number: 148

Date: 29-05-2009 Day number: 149 Date: 30-05-2009 Day number: 150

Date: 31-05-2009 Day number: 151

Observatory: Declination (degrees) 3.59 Rotn 3.40 2386 Jun08 Jul 2387 Aug 2388 Sep 2389 Oct 2390 Nov 2391 Dec 2392 2393 Jan09 2394 Feb 2395 Mar 2396 Apr 2397 May 2398 2399 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) 18869 Rotn 18758 2386 Jun08 Jul 2387 Aug 2388 Sep 2389 Oct 2390 Nov 2391 Dec 2392 2393 Jan09 2394 Feb 2395 Mar 2396 Apr 2397 May 2398 2399 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) -21831 Rotn -21879 2386 Jun08 Jul 2387 Aug 2388 Sep 2389 Oct 2390 Nov 2391 Dec 2392 2393 Jan09 2394 Feb 2395 Mar 2396 Apr 2397 May 2398 2399 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 2009 Daily Mean Declination (deg) 209.0 10min Daily Mean Horizontal Intensity (nt) 18793 50nT Daily Mean Vertical Intensity (nt) -21847 50nT Daily Mean Total Intensity (nt) 28818 50nT Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec

Monthly Mean Values for Port Stanley Observatory 2009 Month D H I X Y Z F January 3 29.8 18810 nt -49 16.6 18775 nt 1147 nt -21851 nt 28832 nt February 3 29.8 18798 nt -49 17.7 18763 nt 1146 nt -21850 nt 28823 nt March 3 28.8 18791 nt -49 18.0 18757 nt 1141 nt -21847 nt 28817 nt April 3 28.5 18786 nt -49 18.3 18752 nt 1139 nt -21845 nt 28812 nt May 3 28.1 nt -49 18.8 18745 nt 1136 nt nt 28806 nt Note i. The values shown here are provisional.