Montserrat Volcano Observatory, Montserrat, West Indies

Scientific Report 88
12 April 1998

This report covers the 14 day period from 00:00 on 29 March to 00:00 (local time) on 12 April, 1998.


Summary

Activity during this reporting period was low. Seismic activity was dominated by volcano-tectonic earthquakes and small rockfalls from the dome.

Visual Observations

Observations during clear periods indicate that no growth of the dome complex has occurred throughout the reporting period. Rockfall activity has been minimal with very small rockfalls occurring down the upper flanks over Gages, the upper flanks of the new dome on the south-west sector of the dome complex and continuing degradation of the steep buttress on the upper flanks of the eastern face. Rockfalls from this buttress were seen travelling down either the gully between the eastern face and the northern flanks (Oct 22 dome) or more commonly down the incised central chute on the eastern flanks. Moderate fumarolic activity was concentrated within this same chute and around the trench between the Boxing Day scar and the fresh dome material on the south-west sector of the dome.

A field team measured the temperature of the pyroclastic flow deposits produced by the September 21 collapse in the area around Trants using a new thermocouple probe on loan from the Cascades Volcano Observatory, USA. A maximum temperature of 357 ?C was recorded at a depth of 2 m within the deposits.

Seismicity

The seismic activity over this period was at a very low level. Numbers of recorded earthquakes were low (Table 1). Earthquake activity consisted principally of volcano-tectonic earthquakes. These events occurred at irregular intervals rather than in swarms. Epicentral solutions for the volcano-tectonic earthquakes show that all of these events occurred below the dome. The number of recorded rockfall signals was also low throughout this period. These events were generally small.

Work was completed on upgrades to the broadband seismic network. The network now consists of 7 stations in total. Two new stations were installed at the South Soufriere Hills and at Mongo Hill, providing increased azimuthal coverage. Both these stations use single vertical component seismometers with corner frequencies of 1 Hz. Radio telemetry was revised for the remaining stations original network.

Table 1: Earthquake types

These earthquake counts are of events that triggered the broadband network's event recording system between 00:00 and 00:00 each day (local time).

Date		VT	Hybrid		LP	Dome RF	LPRF*		HYRF*
29 Mar 98	-	2		2	4	-		-
30 Mar 98	4	-		-	8	-		-
31 Mar 98	1	-		-	5	-		-
1 Apr 98	-	3		-	1	-		-
2 Apr 98	3	2		-	18	-		-
3 Apr 98	6	3		-	11	-		-
4 Apr 98	7	1		-	11	-		1
5 Apr 98	17	2		-	13	-		-
6 Apr 98	4	3		-	19	-		-
7 Apr 98	7	1		1	1	-		-
8 Apr 98	11	-		-	6	-		-
9 Apr 98	16	2		-	3	-		-
10 Apr 98	3	1		-	11	-		-
11 Apr 98	4	-		-	5	-		-

* LPRF: LP earthquake followed by rockfall signal. HYRF: Hybrid earthquake followed by rockfall signal. The LPs, hybrids and rockfalls in these signals are also counted in their respective columns.

Ground Deformation

GPS occupations were made at Whites, Gages, Old Towne, Dagenham, Blakes and Drummonds with the base station at Harris. The summit of Gages Mountain has moved just over 3 cm to the west-north-west since January. This direction is radially away from the dome and is almost identical to the movement direction of the pole to the tilt plane for the tiltmeter on the summit of Gages Mountain. The University of Puerto Rico station at Hermitage shows continued movement to the north-east. The site has moved 15 cm since this time last year with the highest rates of movement occurring since September, 1997.

Volume Measurements

A survey of the dome talus and the deposits in the top of the White River Valley was carried out on the 30th March. This gave a better constrained volume for the talus of 36 million cubic metres, and increases the total dome volume to 120 million cubic metres. The deposits showed an increase of 8.99 million cubic metres, since the previous survey on 17 January 1997. The total volume of the dome and deposits is 300 million cubic metres erupted since November 1995.

Theodolite measurements during a clear window on the 5 April show that the highpoint of the dome complex is the top of the large spine perched near the summit of the fresh material on the south-west sector. This has an elevation of 1031 m and the spine itself has a minimum height of 50 m. Further photos taken from the helicopter combined with GPS positional data were taken on 6 April concentrating on the fresh dome material on the south-west sector to constrain the total dome volume.

Environmental Monitoring

Localities of Dust Trak monitoring sites:

The air quality monitoring programme during this period involved 5 permanent monitoring sites (1-5 below) and three temporary sites (6-8 below). Results are shown in Table 2.

  1. Salem (Old Towne); the Dust Trak on the veranda of the old Montserrat Volcano Observatory (MVO-S). Wind direction was also noted here.
  2. Woodlands, Mango Drive; the Dust Trak on the veranda of a villa.
  3. Woodlands, Palm Loop, Catholic Primary School; the Dust Trak is in the area under the roof where some of the children have classes.
  4. Davy Hill; the Dust Trak is on the veranda of a villa.
  5. St. John's, Mongo Hill; the Dust Trak is on the third floor of the new MVO building with a sampling tube attached and leading out of the window.
  6. Woodlands; Dust Trak on the veranda of a villa near the library.
  7. St. John's / Old Norwood; the Dust Trak is on the veranda of a villa.
  8. Lookout (Secondary School); the Dust Trak is on the concrete corridor outside the school library connected to a solar panel on the roof, during the school Easter holiday.

Table 2 : PM10 (concentration in mg/m3)

These values are approximate 24 hr averages of the PM10 concentration. Aerosol values measured at each of the monitoring sites are accompanied by a note on the level of volcanic activity (VA) and prevailing weather conditions.

Date		1	2	3	4	5	6	7	8	VA	wind	rain	
29th Mar	18	16	19	17	24	-	-	-	Low	320o	PM	
30th Mar	21	23	47	53	21	-	-	-	P	100o	Periodic	
31th Mar	20	27	29	91	18	-	-	-	Low	040o	Overnight	
1st Apr		15	16	29	-	12	-	-	-	Low	040o	AM & overnight	
2nd Apr		9	10	11	36	8	-	-	-	Low	340o	Dry	
3rd Apr		47	12	43	13	11	-	-	-	Low	340o	Evening	
4th Apr		25	23	45	24	10	-	-	-	Low	Still	AM	
5th Apr		32	15	18	18	10	-	-	-	Low	040o	Dry	
6th Apr		16	16	32	52	14	-	-	-	Low	030o	Dry	
7th Apr		60	58	-	100	54	-	-	-	Low	020o	Dry but hazy	
8th Apr		69	48	75	90	24	-	-	-	Low	290o	Evening	
9th Apr		28	24	35	37	-	32	-	-	S	280o	Dry	
10th Apr	25	19	-	32	24	12	27	-	Low	300o	Dry	
11th Apr	15	13	19	22	15	-	8	14	S	290o	Overnight	

P = small plume of ash observed at 06:00 and sulphur smell in St. Peter's.
S = slight increase in volcanic seismicity.
Wind direction was variable during this period

24 Hour averages:
<50 mg m-3	Low
50-100 mg m-3	Raised
100-300 mg m-3	Very High
>300 mg m-3	Alert

Low volcanic activity and occasional rains have generally kept aerosol levels low. Slightly higher aerosol levels were measured on 7th and 8th April and may be due to Saharan dust in the atmosphere. The Davy Hill area, which was affected by traffic jams at the time, showed the highest levels.

MVO Staff Changes

Arrivals:
Willie Aspinall (Aspinall and Associates)
Joe Devine (Brown University/ Seismic Research Unit, Trinidad)
Rob Watts (Bristol University)

Departures:
Wilkie Balgobin (Seismic Research Unit, Trinidad)

Visitors:
Dave Petrie (British Geological Survey)


Montserrat Volcano Observatory