• 제목/요약/키워드: north-south asymmetry

검색결과 21건 처리시간 0.023초

VARIATION IN NORTH-SOUTH ASYMMETRY OF SUN SPOT AREA

  • Chang, Heon-Young
    • Journal of Astronomy and Space Sciences
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    • 제24권2호
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    • pp.91-98
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    • 2007
  • The existence of the North-South asymmetry of the solar activity is widely accepted even though the phenomenon is not yet satisfactorily understood. We have studied the temporal variations in the North-South asymmetry of the sunspot area during the period from May in 1874 to April in 2007. The combined data have been examined for periodicity in the solar activity North-South asymmetry. We have found that (i) solar northern and southern hemispheres show an asymmetric behavior, in terms of a sunspot area, (ii) sunspot areas in northern and southern hemispheres show clearly the 11 year periodicity when they were analyzed separately, as they do when analyzed together, (iii) in addition to the general 11 year periodicity in both northern and southern hemisphere solar activities, there are also noticeable shorter periodicities other than the 11 year periodicity in the asymmetry in North-South activity. Finally, we conclude by pointing out the importance of studying the North-South asymmetry of the solar activity.

Normalized Cross-Correlations of Solar Cycle and Physical Characteristics of Cloud

  • Chang, Heon-Young
    • Journal of Astronomy and Space Sciences
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    • 제36권4호
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    • pp.225-234
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    • 2019
  • We explore the associations between the total sunspot area, solar north-south asymmetry, and Southern Oscillation Index and the physical characteristics of clouds by calculating normalized cross-correlations, motivated by the idea that the galactic cosmic ray influx modulated by solar activity may cause changes in cloud coverage, and in turn the Earth's climate. Unlike previous studies based on the relative difference, we have employed cloud data as a whole time-series without detrending. We found that the coverage of high-level and low-level cloud is at a maximum when the solar north-south asymmetry is close to the minimum, and one or two years after the solar north-south asymmetry is at a maximum, respectively. The global surface air temperature is at a maximum five years after the solar north-south asymmetry is at a maximum, and the optical depth is at a minimum when the solar north-south asymmetry is at a maximum. We also found that during the descending period of solar activity, the coverage of low-level cloud is at a maximum, and global surface air temperature and cloud optical depth are at a minimum, and that the total column water vapor is at a maximum one or two years after the solar maximum.

Latitudinal Distribution of Sunspot and North-South Asymmetry Revisited

  • Chang, Heon-Young
    • Journal of Astronomy and Space Sciences
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    • 제35권2호
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    • pp.55-66
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    • 2018
  • The solar magnetic field plays a central role in the field of solar research, both theoretically and practically. Sunspots are an important observational constraint since they are considered a discernable tracer of emerged magnetic flux tubes, providing the longest running records of solar magnetic activity. In this presentation, we first review the statistical properties of the latitudinal distribution of sunspots and discuss their implications. The phase difference between paired wings of the butterfly diagram has been revealed. Sunspots seem to emerge with the exponential distribution on top of slowly varying trends by periods of ~11 years, which is considered multiplicative rather than additive. We also present a concept for the center-of-latitude (COL) and its use. With this, one may sort out a traditional butterfly diagram and find new features. It is found that the centroid of the COL does not migrate monotonically toward the equator, appearing to form an 'active latitude'. Furthermore, distributions of the COL as a function of latitude depend on solar activity and the solar North-South asymmetry. We believe that these findings serve as crucial diagnostic tools for any potential model of the solar dynamo. Finally, we find that as the Sun modulates the amount of observed galactic cosmic ray influx, the solar North-South asymmetry seems to contribute to the relationship between the solar variability and terrestrial climate change.

태양의 북-남 비대칭성을 고려한 태양활동과 기후변화와의 관계 (On the Relation Between the Sun and Climate Change with the Solar North-South Asymmetry)

  • 조일현;곽영실;조경석;최호성;장헌영
    • Journal of Astronomy and Space Sciences
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    • 제26권1호
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    • pp.25-30
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    • 2009
  • 태양의 북-남 비대칭성을 고려하여 태양활동과 기후변화 사이의 관계에 대하여 연구하였다. 이를 위해 흑점 수와 지구연평균 기온아노말리(temperature anomalies) 시계열을 이용하여 이동 상관계수를 계산하였고 상관계수의 부호가 바뀌는 시점을 태양의 북-남 비대칭성의 부호가 바뀌는 시점과 비교하였다. 상관계수의 부호는 1907년을 기준으로 음의 상관에서 양의 상관으로 바뀌었고 1985년을 기준으로 양의 상관이 을의 상관으로 바뀌었다. 이 둔 시점은 태양의 북-남 비대칭성의 부호가 바뀌는 시점과 잘 일치하였다. 흑점 수에 대한 기온아노말리 변화 그래프를 통해 태양활동과 기후변화 사이의 관계가 1907년과 1985년으로 나뉘어진 세 기간으로 분류되었고 각 기간에 대해서 기온아노말리의 흑점 수에 대한 상관계수를 계산하였다. 이를 통해 태양의 남반구에서 태양활동이 강할 때는 태양활동과 기후변화의 관계가 음의 상관을 보이고 북반구의 태양활동이 강할 때는 양의 상관을 보인다는 것을 확인하였다.

A NEW METHOD FOR NORTH-SOUTH ASYMMETRY OF SUN SPOT AREA ANALYSIS

  • Chang, Heon-Young
    • Journal of Astronomy and Space Sciences
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    • 제24권4호
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    • pp.261-268
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    • 2007
  • We have studied the temporal variation in the North-South asymmetry of the sunspot area during the period from 1874 to 2007. Though the 9-year periodicity is commonly reported, shorter periodicities is still under study. We employ the cepstrum analysis method to analyze the noisy power spectrum of the North-South asymmetry. We demonstrate that the cleaned power spectrum shows reduction of the spurious back-ground noise level. Some of short period peaks in the power spectrum disappear after deconvolution. It should be, however, pointed out that power spectrum might look less noisy because of a filtering process during deconvolution. We conclude by pointing out that a more sophisticate filtering algorithm is required to produce a precise and reliable periodicity estimate.

Solar North-South Asymmetry and Hilbert Transform Analysis

  • Heon-Young Chang
    • 천문학회지
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    • 제56권1호
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    • pp.125-135
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    • 2023
  • Here, we investigated the observed sunspot areas with respect to latitudes using the Hilbert transform technique. Conventional study of the cyclic patterns of sunspots is based on the Lomb-Scargle periodogram, which only obtains the amplitude information. In comparison, our approach characterizes the amplitude as well as the phase of solar activity. We demonstrated the solar North-South asymmetry in the instantaneous amplitude by analyzing daily sunspot data set spanning from the solar cycles 11 to 24. Our findings confirm that the northern hemisphere is dominant in the solar cycles 14, 15, 16, 18, and 20. Unlike the amplitude, the North-South asymmetry in the period of solar activity could not be established. We have also found that the standard deviation as a measure of fluctuation in the phase derivative is minimum in the latitude band 10° < l < 20°, and the fluctuations obtained for latitudes above 30° are considerable.

Acidity in Precipitation and Solar North-South Asymmetry

  • Moon, Ga-Hee;Ha, Kyoung-Yoon;Kang, Seong-Hoon;Lee, Byoung-Ho;Kim, Ki-Beom;Kim, Jung-Hee;Chang, Heon-Young
    • Journal of Astronomy and Space Sciences
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    • 제31권4호
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    • pp.325-333
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    • 2014
  • We are motivated by both the accumulating evidence for the connection of solar variability to the chemistry of nitrogen oxide in the atmosphere and recent finding that the Galactic cosmic-ray (GCR) influx is associated with the solar north-south asymmetry. We have analyzed the measured pH in precipitation over the 109 stations distributed in the United States. We have found that data of pH in precipitation as a whole appear to be marginally anti-correlated with the solar asymmetry. That is, rain seems to become less acidic when the southern hemisphere of the Sun is more active. The acidity of rain is also found to be correlated with the atmospheric temperature, while not to be correlated with solar activity itself. We have carried on the analysis with two subsamples in which stations located in the east and in the west. We find that the pH data derived from the eastern stations which are possibly polluted by sulfur oxides and nitrogen oxides are not correlated with the solar asymmetry, but with the temperature. On the contrary, the pH data obtained from the western stations are found to be marginally anti-correlated with the solar asymmetry. In addition, the pH data obtained from the western stations are found to be correlated with the solar UV radiation. We conclude by briefly pointing out that a role of the solar asymmetry in the process of acidification of rain is to be further examined particularly when the level of pollution by sulfur oxides and nitrogen oxides is low.

북한 핵위협 극복을 위한 한미동맹 효용성: 평가와 대책 (The Efficiency of ROK-U.S. Alliance in Order to Overcome North Korea's Nuclear Threats: Evaluations & Measures)

  • 김연준
    • 융합보안논문지
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    • 제17권2호
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    • pp.89-100
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    • 2017
  • 지난 2017년 1월, 트럼프가 미국의 제 45대 대통령으로 취임하였다. 그는 대선기간 중에 '미국 우선주의'(America First)를 적극적으로 표방하였다. 그의 이런 주장이 대외정책에 있어서 '고립주의'(Isolationism)를 표방하는 것으로 비취지고 있다. 북한의 핵위협에 대하여 미국의 '확장억제'(Extended Deterrenc)에 전적으로 의존하고 있는 한국에 있어서 이는 단순한 문제가 아니다. 즉 미국이 고립주의로 회귀하여 한미동맹 공약이행 의지가 약화되는 것으로 인식될 경우 북한의 오판 가능성은 그만큼 높아질 것이기 때문이다. 그동안 한국사회에서는 미국으로부터 안보를 지원받고 정책적 공조를 제공하는 전형적인 '비대칭 동맹'(Asymmetry Alliance)인 한미동맹의 가치를 재평가하려는 다양한 시도가 있었다. 이에 북한의 고도화된 핵도발 위협에 효과적으로 대응하고, 신장된 한국의 국력수준에 부합된 한미동맹의 효용성을 동맹이론에 입각하여 평가해보고 대책을 강구하였다. 이를 위해 본 연구는 한미동맹을 '자율성-안보 교환 모델'에 기초하여, 위협인식, 정책공조와, 동맹국으로서 가치 측면으로 구체화하여 평가해보고, 향후 한미동맹의 전략적 함의를 도출하였다.

Association between Solar Variability and Teleconnection Index

  • Kim, Jung-Hee;Chang, Heon-Young
    • Journal of Astronomy and Space Sciences
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    • 제36권3호
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    • pp.149-157
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    • 2019
  • In this study, we investigate the associations between the solar variability and teleconnection indices, which influence atmospheric circulation and subsequently, the spatial distribution of the global pressure system. A study of the link between the Sun and a large-scale mode of climate variability, which may indirectly affect the Earth's climate and weather, is crucial because the feedbacks of solar variability to an autogenic or internal process should be considered with due care. We have calculated the normalized cross-correlations of the total sunspot area, the total sunspot number, and the solar North-South asymmetry with teleconnection indices. We have found that the Southern Oscillation Index (SOI) index is anti-correlated with both solar activity and the solar North-South asymmetry, with a ~3-year lag. This finding not only agrees with the fact that El $Ni{\tilde{n}}o$ episodes are likely to occur around the solar maximum, but also explains why tropical cyclones occurring in the solar maximum periods and in El $Ni{\tilde{n}}o$ periods appear similar. Conversely, other teleconnection indices, such as the Arctic Oscillation (AO) index, the Antarctic Oscillation (AAO) index, and the Pacific-North American (PNA) index, are weakly or only slightly correlated with solar activity, which emphasizes that response of terrestrial climate and weather to solar variability are local in space. It is also found that correlations between teleconnection indices and solar activity are as good as correlations resulting from the teleconnection indices themselves.