Information is preliminary and subject to change. All times are local (unless otherwise noted)
Minor fumarolic activity
Minor fumarolic activity continued in June, and an area of recently-killed vegetation was observed on the NNE flank. The Las Pilas complex last erupted 29-31 October 1954, producing explosions from the central crater El Hoyo.
Information Contacts: R. Stoiber and S. Williams, Dartmouth College; M. Carr and J. Walker, Rutgers Univ.; A. Creusot, Instituto Nicaraguense de Energía.
Small vapor plume
In late 1980 a small continuous vapor plume was still being emitted from the top of the kilometer-long crack in the summit.
Information Contacts: R. Stoiber, S. Williams, H.R. Naslund, L. Malinconico, and M. Conrad, Dartmouth College; A. Aburto, D. Fajardo B., Instituto de Investigaciones Sísmicas.
Gas emission continuing from 1952 fissure
The [summit-area] fissure formed in the 1952 eruption was still emitting gas on 16 January 1988. Another small eruption was reported in 1954.
Information Contacts: B. van Wyk de Vries, H. Rymer, and G. Brown, Open Univ; P. Hradecky and H. Taleno, INETER.
Fumarolic activity
An 8-14 µm infrared thermometer was used on 23 April to measure temperatures of the inner wall of the prominent 20-m-deep chasm formed in the [1952] eruption. Weak fumarolic activity was occurring there, and the maximum recorded temperature was 96°C, probably corresponding closely with the gas temperature.
Information Contacts: C. Oppenheimer, Open Univ; B. van Wyk de Vries, INETER.
Continued fumarolic activity; many young prehistoric lava flows
"The El Hoyo fumarole was visited 3 times (15:04) and showed no discernable change from wet- to dry-season conditions (98°C). There is no other strong thermal activity in the summit region of El Hoyo.
"The central crater walls of El Hoyo (150 m deep) are composed of lava and agglutinated spatter, probably produced by Hawaiian activity (figure 1). In contrast, Las Pilas, Asososca, and Cerro Negro are predominantly scoria cones formed by Strombolian eruptions. All vents have produced extensive lava flows. Poorly vegetated flows extend up to 15 km from both Las Pilas and El Hoyo and are probably less than a few thousand years old."
Reference. Bice, D.C., 1980, Tephra stratigraphy and physical aspects of recent volcanism near Managua, Nicaragua: Ph.D. Dissertation, Univ of California, Berkeley, 422 p.
Information Contacts: B. van Wyk de Vries, O. Castellón, A. Murales, and V. Tenorio, INETER.
Small gas plume
A persistent, very small gas plume was visible in late April, rising from the NE margin of the 1-km fissure formed in 1952. Weak activity has been reported from this fumarole since 1980.
Information Contacts: S. Williams, Arizona State Univ.
Weak fumarolic activity
El Hoyo's main fumarole was emitting vapor at usual levels on 6-7 January.
Information Contacts: Andrea Borgia, Instituto Nazionale di Geofisica, via di Vigna Murata 605, 00143 Roma, Italy; B. van Wyk de Vries, Open Univ; Peter J. Baxter, Dept of Community Medicine, Fenner's, Gresham Road, Cambridge, England.
Weak fumarolic activity
A continuous white plume from El Hoyo was easily visible at distances of 5-10 km from the volcano throughout the entire first week of September.
Information Contacts: Michael Conway and Andrew Macfarlane, FIU; Charles Connor, CNWA Bldg. 168, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228-0510; Oscar Leonel Urbina and Cristian Lugo, INETER.
Dense white plumes issue from a 10-m-diameter pit crater
On 6 March 1994, we visited Las Pilas to determine the source and nature of a dense white plume, visible for at least 10 km to the S, that rose from the upper S slope of the volcano. The plume, which smelled strongly of sulfur, emerged from the bottom of a small phreatic (?) pit crater. The crater measured roughly 10 m in diameter and 5-10 m deep. The pit walls were vertical, and the pit opening was mantled by a thin coating of native sulfur. Extensive mixing with atmospheric gases occurred before the plume rose from the pit. Immediately downslope from the crater there appeared to be bedded volcanic deposits. Their presence suggests that the pit crater was the source of numerous phreatic-phreatomagmatic explosions.
We briefly examined a large, circular phreatic pit crater 50-75 m W of the small phreatic pit. This larger crater was about 30-40 m in diameter, and roughly 30 m deep. The phreatic explosion that produced the crater must have been unusually powerful, because it disrupted several (5-7 m thick) basaltic lava flows. No fumarolic activity was observed at this crater, and we saw no evidence of surge deposits in its vicinity. A Hewlett Packard chromatograph of in-situ soils at Las Pilas yielded 0.19 and 0.21 vol. % CO2, values probably within the range of background in local volcanic soils (0.04-0.1 vol.%).
CO2 in soils at volcanic areas varies considerably, and includes some relatively high values. A preliminary survey of the literature suggests soil gas CO2 in volcanic areas ranges from ten to several-hundred times the background found in many non-volcanic areas.
Information Contacts: Cristian Lugo, Instituto Nicaraguense de Estudios Territoriales (INETER), Apartado 17610-2110, Managua, Nicaragua; Michael Conway, Andrew Macfarlane, and Peter LaFemina, Florida International Univ (FIU), Miami, FL 33199 USA; John B. Murray, Ben van Wyk de Vries, and Adam Maciejewski, Open Univ, Milton Keynes, MK7 6AA, U.K..