Montserrat Volcano Observatory, Montserrat, West Indies

Scientific Report 87
29 March 1998

This report covers the 14 day period from 00:00 on 15 March to 00:00 (local time) on 29 March 1998.


Summary

The level of seismic and volcanic activity during the reporting period was very low. There was no evidence for dome growth and rockfall activity was minimal. Deformation of the northern and eastern flanks continued.

Visual Observations

The appearance of the dome did not change much throughout the reporting period apart from a slight degradation of the upper flanks and the continued development of small rockfall chutes on the eastern and south western flanks of the dome. There were few rockfalls during the reporting period and most of these were small and caused by degradation of the dome. The disintegration of a steep rocky buttress in the dome complex above the Tar River valley produced several small pyroclastic flows. The largest of these was observed by a field team at Windy Hill, it travelled down a narrow ravine and reached as far as the Tar River Estate house. There were also some small rockfall deposits below the area of fumarolic activity on the eastern flanks of the dome complex. Ash venting was absent throughout this period.

Seismicity

Seismic activity over this period remained at a very low level. Numbers of recorded earthquakes were low. Epicentral solutions suggest that all the earthquake activity is still concentrated below the area of the dome. Similarly there were very few dome rockfalls and the size of these events was small.

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*

15 Mar 98	6	1	-	3	-	-
16 Mar 98	1	2	-	8	-	-
17 Mar 98	5	11	-	12	-	-
18 Mar 98	11	3	-	4	-	-
19 Mar 98	1	7	1	10	-	-
20 Mar 98	-	5	1	7	1	-
21 Mar 98	4	1	-	7	-	-
22 Mar 98	4	5	-	5	-	-
23 Mar 98	6	6	1	8	-	-
24 Mar 98	8	12	3	3	-	-
25 Mar 98	2	2	-	4	1	-
26 Mar 98	1	1	-	5	-	-
27 Mar 98	1	-	-	1	-	-
28 Mar 98	-	3	-	2	-	-

*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 of Blakes, Drummonds, Old Towne and Dagenham were made during the reporting interval, running the new base station at Harris. The sites appear stable with respect to Harris. Data from the University of Puerto Rico station at Hermitage show that that site is still moving to the north east.

The new reflector on Peak B was shot four times during the reporting interval, although the line continues to shorten (8cm total shortening since January 25th 1998), the last two measurements suggest the shortening rate may be slowing slightly.

Volume Measurements

There are no volume measurements to report for this time period. There have been no observations to suggest that the dome is still growing, and therefore we can assume that growth has ceased for the time being.

Environmental Monitoring

The air quality monitoring programme during this period involved 5 permanent monitoring sites and one temporary site. These were located at:

  1. Cavalla Hill; the Dust Trak on the veranda at the back of the villa.
  2. Salem (Old Towne); the Dust Trak on the veranda of the old Montserrat Volcano Observatory (MVOsouth). Wind direction was also noted here.
  3. Woodlands, Mango Drive; the Dust Trak on the veranda of a villa.
  4. Woodlands, Palm Loop, Catholic Primary School; the Dust Trak is in the area under the roof where some of the children have classes.
  5. St. Peter's, Cheapend, St. Peter's Place; the Dust Trak is on the balcony of a villa.
  6. St. John's, Mongo Hill; the dust trak is on the third floor of the MVO building with a sampling tube attached and leading out of the window.
  7. Davy Hill; the Dust Trak is on the veranda of a villa.

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	VA	wind		rain	other	
15-Mar	-	75	63	54	83	36	-	Low	320  Breezy   	Dry		
16-Mar	75	64	60	76	44	35	-	Low	290  Breezy	Dry	Holiday	
17-Mar	65	68	61	81	38	31	-	Low	300  Breezy	am	Holiday	
18-Mar	29	54	24	36	17	48	13	Low	300  Breezy	Periodic		
19-Mar	18	23	15	31	8	33	7	Low	N-S  Gusts	am,eve		
20-Mar	20	23	16	45	15	29	7	Low	Light		Night		
21-Mar	19	25	16	17	15	26	7	Low	280  Moderate	Night		
22-Mar	24	32	21	25	-	29	12	Low	300  Gusty	dry		
23-Mar	21	24	18	52	-	30	22	Low	290  Breezy 	am		
24-Mar	50	44	43	70	-	56	-	Low	310-320 Breezy	am		
25-Mar	20	27	17	39	-	27	16	S	280  Light	dry		
26-Mar	-	10	8	37	-	21	8	Low	N-S  Light	Periodic		
27-Mar	-	16	14	42	-	25	13	Low	300  Moderate	pm		
28-Mar	-	23	17	22	-	29	18	Low	300  Strong	Night		
29-Mar	-	18	16	19	-	24	17	Low	320  Light	pm		

S = increase in volcanic seismicity overnight.

Low volcanic activity and occasional rains have generally kept aerosol levels low. Although volcanic activity was low, there was a small increase in volcanic seismicity between 10pm on 23rd March and 4am on 24th march. This coincides with comparatively higher aerosol concentrations on Tuesday 24th march.

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
MVO Staff Changes

Departures:
Richard Luckett (British Geological Survey)

Visitors
Peter Day (British Geological Survey)
Dawn Pirie (Edinburgh University)
Dave Stewart (British Geological Survey)


Montserrat Volcano Observatory